<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">JMP</journal-id><journal-title-group><journal-title>Journal of Modern Physics</journal-title></journal-title-group><issn pub-type="epub">2153-1196</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/jmp.2021.1212098</article-id><article-id pub-id-type="publisher-id">JMP-112694</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  A New Physics Would Explain What Looks Like an Irreconcilable Tension between the Values of Hubble Constants and Allows &lt;i&gt;H&lt;sub&gt;0&lt;/sub&gt;&lt;/i&gt; to Be Calculated Theoretically Several Ways
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Claude</surname><given-names>Mercier</given-names></name><xref ref-type="aff" rid="aff1"><sub>1</sub></xref></contrib></contrib-group><aff id="aff1"><label>1</label><addr-line>Independent Researcher, Baie-Comeau, Canada</addr-line></aff><pub-date pub-type="epub"><day>09</day><month>10</month><year>2021</year></pub-date><volume>12</volume><issue>12</issue><fpage>1656</fpage><lpage>1707</lpage><history><date date-type="received"><day>1,</day>	<month>September</month>	<year>2021</year></date><date date-type="rev-recd"><day>23,</day>	<month>October</month>	<year>2021</year>	</date><date date-type="accepted"><day>26,</day>	<month>October</month>	<year>2021</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
   Observing galaxies receding from each other, Hubble found the universe’s expansion in 1929. His law that gives the receding speed as a function of distance implies a factor called Hubble constant <em>H</em><sub><em>0</em></sub>. We want to validate our theoretical value of <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> ≈ 72.09548580(32) km&amp;sdot;s<sup>-</sup><sup>1</sup>&amp;sdot;MParsec<sup>-1</sup> with a new cosmological model found in 2019. This model predicts what may look like two possible values of <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub>. According to this model, the correct equation of the apparent age of the universe gives ~ 14.14 billion years. In approximation, we get the well-known equation 1/<em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> ≈ 13.56 billion years. When we force these ages to fit the 1/<em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> formula, it gives two different Hubble constant values of ~69.2 and 72.1 km&amp;sdot;s<sup>-1</sup>&amp;sdot;sdot;MParsec<sup>-1</sup>. When we apply a theoretical correction factor of <em>η</em> ≈ 1.042516951 on the first value, both target the second one. We found 42 equations of <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> linking different physics constants. Some are used to measure <em style="white-space:normal;">H</em><sub style="white-space:normal;"><em>0</em></sub> as a function of the average temperature<em> T</em> of the Cosmological Microwave Background and the universal gravitational constant <em>G</em>:  
   <em>H</em><sub><em>0</em></sub> ≈ 72.06(90) km&amp;sdot;s-<sup>1</sup>&amp;sdot;MParsec<sup>-1</sup> from <em>T </em>by Cobra probe &amp; Equation (16)  
   <em>H</em><sub><em>0</em></sub> ≈ 71.95(50) km&amp;sdot;s<sup>-1</sup>&amp;sdot;MParsec<sup>-1 </sup>from<em> T</em> by Partridge &amp; Equation (16)  
   <em>H</em><sub><em>0</em></sub> ≈ 72.086(36) km&amp;sdot;s<sup>-1</sup>&amp;sdot;MParsec<sup>-1 </sup>from <em>G</em> &amp; Equation (34)  
   <em>H</em><sub><em>0</em></sub> ≈ 72.105(36) km&amp;sdot;s<sup>-1</sup>&amp;sdot;MParsec<sup>-1</sup> from <em></em><em>G</em> &amp; Equations (74), (75), or (76). With 508 published values, <em>H</em><sub><em>0</em></sub> ≈ 72.0957 &#177; 0.33 km&amp;sdot;s<sup>-1</sup>&amp;sdot;MParsec<sup>-1</sup> seems to be the “ideal” statistical result. It validates our model and our theoretical <em>H</em><sub><em>0</em></sub> value which are useful to find various interactions with the different constants. Our model also explains the ambiguity between the different universe’s age measurements and seems to unlock a tension between two <em>H</em><sub><em>0</em></sub> values. 
 
</p></abstract><kwd-group><kwd>Hubble Constant &lt;i&gt;H&lt;sub&gt;0&lt;/sub&gt;&lt;/i&gt;</kwd><kwd> Hubble Tension</kwd><kwd> Age of the Universe</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>In astrophysics, the Hubble constant H<sub>0</sub> [<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>] is a parameter to analyze the universe. Nevertheless, it is also one of the lesser-known values.</p><p>In 1916, Einstein found the general relativity laws [<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]. His equations expect that the universe is either expanding or in a Big Crunch. He could have been the first to predict the universe’s expansion, but influenced by the popular idea, Einstein forced his model to be static with a cosmological constant Λ. In 1922, Friedmann showed from relativity that the universe expands at a calculable rate [<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]. In 1927, Georges Lemaitre published independent research [<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>], giving what is now known as Hubble’s law. In 1929, Hubble discovered the universe’s expansion [<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]. Equation (1) gives Hubble’s law, with v being the receding speed in km·s<sup>−1</sup>, D being the distance between the observed object and the observer, and H<sub>0</sub> being the Hubble constant. He measured about H<sub>0</sub> ≈ 500 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. His high value was due to a wrong calibration of the cepheids used to evaluate distances. Hubble’s law was correct, but H<sub>0</sub> was remaining to be found with accuracy.</p><p>v = D H 0 (1)</p><p>Physicists get H<sub>0</sub> based on far cosmic objects (Cepheids, supernovae, red giants, etc.) or local measurements (CMB, universal gravitational constant G, etc.). Including error margins of published values (see the software in Annex A), H<sub>0</sub> is between 19 to 174 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. However, two values are often measured ~69.2 and ~72.1 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. An irreconcilable tension between some H<sub>0</sub> values shows up [<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>]. Even with good accuracies, their error margins do not always overlap. It may let us think that only one of these values is right. No one considered it possible that both values may be in some way correct.</p><p>In 2019, we wrote an article [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>] explaining what may look like two values for H<sub>0</sub>. We calculated the universe age, obtained a result of complex type, and an apparent age of the universe of ~14.4 billion years. The complete equation may be approximated by 1/H<sub>0</sub>, giving ~13.56 billion years. We notice that there is a difference of ~4.25% between the approximated and the non-approximated values.</p><p>Cosmologists use 1/H<sub>0</sub> to calculate the universe’s age. Thus, if we could measure the apparent age of the universe with no approximation, we would conclude wrongly that the Hubble constant is ~4.25% lower than it should be.</p><p>We hypothesize that two values of H<sub>0</sub> are somehow obtained from an approximated and non-approximated equation of the apparent age of the universe. The confusion leads to a tension between two values when there should be only one.</p><p>We summarize our cosmological model [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>] to get H<sub>0</sub> as a function of α, c, and r<sub>e</sub>. We found ways to measure H<sub>0</sub> locally by using the Cosmological Microwave Background (CMB) temperature T and by using the universal gravitational constant G [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref7">7</xref>]. Based on our model, we found a theoretical equation to calculate H<sub>0</sub> from CODATA values (Committee of Data for Science and Technology) [<xref ref-type="bibr" rid="scirp.112694-ref8">8</xref>].</p><p>H 0 = c α 19 β r e ≈ 72.09548580 ( 32 )     km ⋅ s − 1 ⋅ MParsec − 1 where β = 3 − 5 ≈ 0.76 (2)</p><p>We want to validate this theoretical value of H<sub>0</sub> and highlight the tension between two measured values of H<sub>0</sub>. We list the results of the most recent measures of H<sub>0</sub> and build a graph showing someway the popularity of each H<sub>0</sub> value range.</p><p>We list 42 H<sub>0</sub> equations. Certain overcome the difficulties to do experimental measurements. We use one of them as a third measurement of H<sub>0</sub>. Our cosmological model shows that H<sub>0</sub> and the speed of light are not constant.</p></sec><sec id="s2"><title>2. Physics Parameters</title><p>A compact form of notation is used to display tolerances (i.e., 2.734(10) K means 2.734 &#177; 0.010 K). The CODATA 2014 [<xref ref-type="bibr" rid="scirp.112694-ref8">8</xref>] is used to compare the results of our new equations with the articles published in 2019 and 2020.</p><p>Light speed in a vacuum c = 2 99792458   m ⋅ s − 1</p><p>Permeability of free space μ 0 = 4 π &#215; 10 − 7     NA − 2</p><p>Permittivity of free space ε 0 ≈ 8.854187817 &#215; 10 − 12     F ⋅ m − 1</p><p>Universal gravitational constant G ≈ 6.67408 ( 31 ) &#215; 10 − 11     m 3 ⋅ kg − 1 ⋅ s − 2</p><p>Electron rest mass m e ≈ 9.10938356 ( 11 ) &#215; 10 − 31   kg</p><p>Classical electron radius r e ≈ 2.8179403227 ( 19 ) &#215; 10 − 15   m</p><p>Electron charge q e ≈ − 1.6021766208 ( 98 ) &#215; 10 − 19     C</p><p>Planck length L p ≈ 1.616229 ( 38 ) &#215; 10 − 35   m</p><p>Planck time t p ≈ 5.39116 ( 13 ) &#215; 10 − 44   s</p><p>Planck mass m p ≈ 2 .176470 ( 51 ) &#215; 10 − 8     kg</p><p>Planck constant h ≈ 6.626070040 ( 81 ) &#215; 10 − 34     J ⋅ s</p><p>Fine-structure constant α ≈ 7.2973525664 ( 17 ) &#215; 10 − 3</p><p>Boltzmann constant k b ≈ 1.38064852 ( 79 ) &#215; 10 − 23   J ⋅ K − 1</p><p>Rydberg constant R ∞ ≈ 10973731.568508 ( 65 )   m − 1</p></sec><sec id="s3"><title>3. Summary of our Theory</title><p>Our theory is based on a cosmological model officially shown in 2019 [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>], but it summarizes papers we wrote at www.pragtec.com/physique since 2011. First, we outline some main milestones as we did in 2020 [<xref ref-type="bibr" rid="scirp.112694-ref7">7</xref>].</p><sec id="s3_1"><title>3.1. Our Cosmological Model</title><p>We hypothesize that there was one expanding sphere containing all matter at the Big Bang. There was no light. After ~360000 years [<xref ref-type="bibr" rid="scirp.112694-ref9">9</xref>], electrons became free to move because of a lower density universe, and the light appeared and began to travel through space, creating a 4-D expanding sphere called the “luminous universe”. As the matter cannot travel as fast as light [<xref ref-type="bibr" rid="scirp.112694-ref10">10</xref>], it created a smaller 4-D expanding sphere, the “material universe”, imbricated in the “luminous universe”.</p><p>Einstein found that the presence of a massive object reduces the speed of light v<sub>L</sub> [<xref ref-type="bibr" rid="scirp.112694-ref11">11</xref>]. Schwarzschild calculated v<sub>L</sub> in a context of a weak gravitational field Φ using general relativity [<xref ref-type="bibr" rid="scirp.112694-ref12">12</xref>]. With |Φ| &lt;&lt; c<sup>2</sup> around a spherical mass, Equation (3) gives v<sub>L</sub> as a function of c and a local refractive index n<sub>0</sub> (function of G [<xref ref-type="bibr" rid="scirp.112694-ref13">13</xref>] ).</p><p>v L ( r ) = c n 0 where n 0 = 1 − 2 Φ / c 2 1 + 2 Φ / c 2 and Φ = − G m r ≤ 0 (3)</p><p>From an observer on Earth, c seems constant. However, the knowledge of a precise value of c dates only from 19 century [<xref ref-type="bibr" rid="scirp.112694-ref14">14</xref>]. In 1929, Edwin Hubble found that the universe is expanding [<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]. As the apparent universe radius increases, the density of this latest must decrease over time, causing the refractive index of the vacuum to drop. As a result, it causes light to accelerate slowly.</p><p>In Equation (3), c is the local speed limit for light in a vacuum in our universe area. Admitting that light accelerates while the universe expands, it will tend towards another asymptotical speed limit k affected by a local refractive index n. For now, k is unknown. Let us build Equation (4), which is analog to Equation (3) for the universe [<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]. Our universe parcel is at a distance r<sub>u</sub> from the universe’s apparent mass center m<sub>u</sub>. The local speed of light c results from Equation (4).</p><p>c = k n where n = 1 − 2 Θ / k 2 1 + 2 Θ / k 2 and Θ = − G m u r u ≤ 0 (4)</p><p>Similarly to r<sub>u</sub>, the R<sub>u</sub> value is the apparent radius of curvature of the luminous universe [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref15">15</xref>] (also called Hubble radius [<xref ref-type="bibr" rid="scirp.112694-ref16">16</xref>] ). It is a function of c and H<sub>0</sub>. It is “apparent” since Equation (5) assumes c constant for a time equal to the universe’s age. Now, its speed is c, but it is not constant in our model [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>]. It was lower in the past and will increase while the universe expands. The H<sub>0</sub> value represents the expansion rate of the material universe in km·s<sup>−1</sup>·MParsec<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]. It is the local derivative of the velocity of matter v m with respect to the element of distance dr.</p><p>H 0 = d v m d r | r = r u = β c r u = β c β R u ⇒ R u = c H 0 (5)</p><p>Locally, at a distance r = r<sub>u</sub>, matter recedes radially from the center of mass of the universe at a rate β times slower than the speed of light c.</p><p>r u = β R u = β c H 0 (6)</p><p>The apparent mass m<sub>u</sub> of the universe is given by Equation (7) [<xref ref-type="bibr" rid="scirp.112694-ref15">15</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref17">17</xref>]:</p><p>m u = c 3 G H 0 = R u c 2 G (7)</p><p>Our universe parcel is at a distance r<sub>u</sub> from the center of the mass m<sub>u</sub>. It travels at a speed v<sub>m</sub> relative to this latest. The ratio β is the asymptotical speed of light k in a vacuum (when R<sub>u</sub> tends towards infinity) influenced by a refractive index n that is itself influenced by a gravitational potential Θ.</p><p>v m = β k n where n = 1 − 2 Θ / k 2 1 + 2 Θ / k 2 and Θ = − G m u r u (8)</p><p>Hubble measured H<sub>0</sub> from the global movement of galaxies at our location [<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>], at r<sub>u</sub>. They have their own movement. As the universe expands, they are generally moving away from each other. The derivative of the material universe speed v<sub>m</sub> according to the element of distance dr evaluated at r = r<sub>u</sub> is H<sub>0</sub> [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>].</p><p>H 0 = d v m d r | r = r u = k β y r u ( 1 ( 1 + y ) 1 − y 2 ) where y = 2 G m u k 2 r u (9)</p><p>Solving Equations (4) to (7), and (9) gives Equations (10) to (14) [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>]. The expending speed ratio β between the material and the luminous universes is geometric. It is also the ratio between r<sub>u</sub> and R<sub>u</sub>. It is unique to our model and essential to depict many constants and make links between the infinitely large and small in the Dirac hypothesis on large numbers [<xref ref-type="bibr" rid="scirp.112694-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref19">19</xref>].</p><p>k = c 2 + 5 ≈ 6.17 &#215; 10 8     m ⋅ s − 1 (10)</p><p>β = 3 − 5 ≈ 0.764 (11)</p><p>R u ≈ 1.28 &#215; 10 26     m (12)</p><p>r u ≈ 9.80 &#215; 10 25     m (13)</p><p>m u ≈ 1.73 &#215; 10 53     kg (14)</p></sec><sec id="s3_2"><title>3.2. Our First Method to Measure H<sub>0</sub> as a Function of T (from CMB)</title><p>The accuracies of m<sub>u</sub>, r<sub>u</sub>, and R<sub>u</sub> widely depend on H<sub>0</sub> which could be between 19 and 174 km·s<sup>−1</sup>·MParsec<sup>−1</sup> (listed in the software in Annex A). Therefore, a better method of measuring H<sub>0</sub> is required to know m<sub>u</sub>, r<sub>u</sub>, and R<sub>u</sub> more accurately.</p><p>We calculated the CMB temperature T as a function of H<sub>0</sub> and G [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>]. This equation considers the universe as an ideal black body since it would absorb any incident radiation coming from outside, and it does not reflect or transmit any form of energy outside of the luminous universe (since it expands at the speed of light).</p><p>T = β k b ( 15 α 2 h 3 c 5 H 0 2 8 π 6 G ) 1 / 4 (15)</p><p>Let us isolate H<sub>0</sub> from Equation (15). The accuracy mainly depends on the CMB temperature T. Using T ≈ 2.736(17) K (from Cobra probe [<xref ref-type="bibr" rid="scirp.112694-ref20">20</xref>] ), we get.</p><p>H 0 ( T ) = π 3 T 2 k b 2 β 2 α 8 G 15 c 5 h 3 ≈ 72.06 ( 90 )   km ⋅ s − 1 ⋅ MParsec − 1 (16)</p><p>with Partridge T ≈ 2.734(10) K, and H<sub>0</sub> ≈ 71.95(50) km·s<sup>−1</sup>·MParsec<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.112694-ref21">21</xref>]. As the least accurate value is T, Equation (16) measures H<sub>0</sub> from the CMB temperature. These values lead to new links and are in our software in Annex A.</p></sec><sec id="s3_3"><title>3.3. Dirac Hypothesis about Large Numbers</title><p>Dirac found (inaccurately) that large numbers come into a few orders of magnitude with same dimensions quantities ratios [<xref ref-type="bibr" rid="scirp.112694-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref19">19</xref>]. All ratios come from N, via certain factors [<xref ref-type="bibr" rid="scirp.112694-ref22">22</xref>]. It represents the maximum number of photons in the universe. We get the highest number when the associated mass m<sub>ph</sub> of a photon is the smallest. This happens when the energy of the photons is at its lowest and with a wavelength of the same length as the circumference of the luminous universe (i.e., 2πR<sub>u</sub>) [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>]. Let us calculate m<sub>ph</sub> by equating its corpuscular and wave energies.</p><p>m p h c 2 = h c 2 π R u ⇒ m p h = h 2 π R u c ≈ 2.74 &#215; 10 − 69     kg (17)</p><p>We get N by dividing the apparent mass m<sub>u</sub> of the universe (Equation (7)) by the mass m<sub>ph</sub> associated with a photon of 2πR<sub>u</sub> wavelength (Equation (17)).</p><p>N = m u m p h = 2 π c 5 h G H 0 2 ≈ 6.3018 ( 62 ) &#215; 10 121 (18)</p><p>If we try to make a precise evaluation of N by using the Equations (6), (7), (16), and (17), we obtain Equation (19) which is dependent mainly on T. We evaluate the result by using the CODATA 2014 [<xref ref-type="bibr" rid="scirp.112694-ref8">8</xref>] and the average CMB temperature from Cobra probe [<xref ref-type="bibr" rid="scirp.112694-ref20">20</xref>]. Finally, we note that N is dimensionless as α.</p><p>N = 15 h 2 α 2 β 4 c 10 4 π 5 G 2 k b 4 T 4 ≈ 6.31 ( 15 ) &#215; 10 121 (19)</p><p>Assuming α used as a scale factor applied a few times, we postulate Equation (20). It seems impossible to get this equation from standard physics [<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>].</p><p>POSTULATE#1: N = 1 / α 57 ≈ 6.303419702 ( 84 ) &#215; 10 121 (20)</p><p>In the next formulas, Planck temperature is T<sub>p</sub> ≈ 1.42 &#215; 10<sup>32</sup> K. This is the highest temperature reached at the Big Bang. It happens when we put the entire mass m<sub>u</sub> in a point-like pellet of Planck length radius L<sub>p</sub>. Planck charge is given by q<sub>p</sub> ≈ 1.88 &#215; 10<sup>−18</sup> C.</p><p>“Large” numbers are obtained with N exponent a fraction, such as N<sup>1/2</sup>, N<sup>1/3</sup>, N<sup>1/4</sup>, … N<sup>1/57</sup>, etc. We get these in different ways by using various parameters of the universe [<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]. They are always unitless. Some come from Dirac’s hypothesis on large numbers [<xref ref-type="bibr" rid="scirp.112694-ref18">18</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref19">19</xref>]. Some links will be used later [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>].</p><p>N 2 / 3 = m u α m e β 1 / 2 = R u 2 β r e 2 = m p 4 α 4 m e 4 β 2 = m e 2 β m p h 2 α 2 ≈ 1.58 &#215; 10 81 (21)</p><p>N 1 / 2 = m p m p h = R u L p = 1 t p H 0 = 2 π T p k b h H 0 = − 1 q e 4 π m u R u α μ 0 ≈ 7.94 &#215; 10 60 (22)</p><p>N 1 / 3 = m u r e α m e R u β = m e β m p h α = R u β r e = α q e 2 4 π ε 0 G β m e 2 ≈ 3.99 &#215; 10 40 (23)</p><p>N 1 / 4 = T p T ( 15 β 4 α 2 π 3 ) 1 / 4 = k b T m p h c 2 ( π 3 15 β 4 α 2 ) 1 / 4 ≈ 2.82 &#215; 10 30 (24)</p><p>N 1 / 6 = r e L p β = m p α m e β = α 3 4 π R ∞ L p β = 2 π r e k b T p h c β ≈ 1.99 &#215; 10 20 (25)</p><p>N 1 / 16 = ( 4 π c R ∞ β H 0 ) 57 / 256 = ( β T p T ) 1 / 4 ( 15 α 2 π 3 ) 1 / 16 ≈ 4.10 &#215; 10 7 (26)</p><p>N 1 / 19 = 1 4 π R ∞ r e = ( β m e 2 m p h 2 ) 1 / 12 = 16 π 2 β L p R u R ∞ 2 α ≈ 2.57 &#215; 10 6 (27)</p><p>N 1 / 57 = q p 2 q e 2 = ( m p 2 m e 2 β ) 1 / 21 = ( q e 2 4 π β ε 0 G m e 2 ) 1 / 20 = 1 α ≈ 137 (28)</p><p>In a non-published document [<xref ref-type="bibr" rid="scirp.112694-ref22">22</xref>], we show over 150 links that give N with various parameters. The universe is well-linked between the infinitely large and the infinitely small. Almost everything changes while the universe is expanding.</p></sec><sec id="s3_4"><title>3.4. Precise Calculation of H<sub>0</sub></title><p>Unlike Equation (16), we look for an equation that does not use G and T to get H<sub>0</sub> since they do not have good accuracies. Usually, G intervenes in the calculations of gravitational force and energy. Without any details (see [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref7">7</xref>] ), let us calculate the electrical energy E<sub>e</sub> between two electrons separated by a space equal to the classical electron radius r<sub>e</sub>. The electrical energy E<sub>e</sub> is not linked to the distance since we get E e = m e c 2 . We evaluate the gravitational energy for the same conditions, finding E g = G m e 2 / r e . If these experiments are done at the luminous universe periphery, we get an electrical energy E ′ e = E e and a gravitational energy E ′ g = E g / β . The ratio between E ′ e and E ′ g gives Equation (29).</p><p>E ′ e E ′ g = m e c 2 ( G m e 2 β r e ) = c 2 r e G m e β ≈ 5.45 &#215; 10 42 (29)</p><p>As in Equation (20), we realize that the fine-structure constant α plays a role in determining orders of magnitude. By adjusting the exponent of the fine-structure constant α, we obtain a result identical to Equation (29).</p><p>1 α 20 ≈ 5.45 &#215; 10 42 (30)</p><p>Equations (29) and (30) seam equal. By isolating G, we get an equation that becomes postulate #2. We cannot deduce this equation from standard physics.</p><p>POSTULATE#2: G = c 2 r e α 20 m e β ≈ 6.673229809 ( 86 ) &#215; 10 − 11     m 3 ⋅ kg − 1 ⋅ s − 2 where β = 3 − 5 (31)</p><p>We associate the wave energy with the energy of the electron mass m<sub>e</sub>.</p><p>m e c 2 = h c α 2 π r e (32)</p><p>with Equations (20), (31), and (32), we get Equation (33).</p><p>H 0 = c α 19 β r e ≈ 72.09548580 ( 32 )   km ⋅ s − 1 ⋅ MParsec − 1 (33)</p><p>This value is like Soltis with 72.1 &#177; 2.0 km·s<sup>−1</sup>·MParsec<sup>−1</sup>, Martinelli’s with 72 . 1 − 1.8 + 2.1 km·s<sup>−1</sup>·MParsec<sup>−1</sup>, and Salvatelli’s with 72 . 1 − 2.3 + 3.2 km·s<sup>−1</sup>·MParsec<sup>−1</sup> (see the list of value in our software in Annex A). Our theoretical value seems to make sense.</p></sec><sec id="s3_5"><title>3.5. Our Second Method to Measure H<sub>0</sub> as a Function of G</title><p>We want to find a second way to measure H<sub>0</sub> as a function of G. We must use accurate parameters, such as α and the characteristics of the electron (m<sub>e</sub> and r<sub>e</sub>). We look for an equation dependent on G without any rational exponent that reduces the sensitivity. We can use Equations (31) and (33). From each of them, we isolate r<sub>e</sub>, and we make both equal to get H<sub>0</sub>. Since G is the least precise value, Equation (34) evaluates H<sub>0</sub> as a function of G. We used CODATA 2014 values.</p><p>H 0 = c 3 α 39 G m e β ≈ 72.086 ( 36 )   km ⋅ s − 1 ⋅ MParsec − 1 (34)</p><p>This result is about 25 times more precise than Equation (16) that uses the average CMB temperature T. We included this result in our software in Annex A.</p></sec></sec><sec id="s4"><title>4. Hubble Constant versus the Age of the Universe</title><p>We calculate the universe’s age with our cosmological model to understand what seems to be two potential values of H<sub>0</sub>. We measure H<sub>0</sub> by observing cosmological objects. Universe’s age Δt<sub>u</sub> is of complex type and results from the integral of the inverse of the expanding speed of the material universe v<sub>m</sub> with the element of distance dr evaluated between the universe’s center of mass (at r = 0) and the apparent material universe radius of curvature at our location r<sub>u</sub>.</p><p>Δ t u = ∫ r = 0 r = r u 1 v m ( r ) d r = Δ t h u + Δ t 0 h (35)</p><p>The Δt<sub>hu</sub> is the time elapsed between the horizon (r = r<sub>h</sub>) and here (r = r<sub>u</sub>):</p><p>Δ t h u = ∫ r = r h r = r u 1 v m ( r ) d r ( Realtyperesult ) (36)</p><p>The Δt<sub>0h</sub> is the elapsed time between r = 0 and the horizon r = r<sub>h</sub>:</p><p>Δ t 0 h = ∫ r = 0 r = r h 1 v m ( r ) d r ( Imaginarytyperesult ) (37)</p><p>At the universe horizon r = r<sub>h</sub>, the speed of light is zero. We cannot see beyond the horizon. The delay Δt<sub>hu</sub> is the time elapsed between the horizon h and our actual position r<sub>u</sub> in the universe. The delay Δt<sub>0h</sub> is the time elapsed between the center of mass of the universe and the horizon r<sub>h</sub> (given by Equation (38)).</p><p>r h = 2 G m u k 2 (38)</p><p>Performing the integral calculation of Equation (35), we get Equation (39).</p><p>∫ 1 v m ( r ) d r = ( z ( r ) + 2 G ⋅ m u ln ( 2 [ k 2 r + z ( r ) ] ) ) β k 3 where     z ( r ) = k 4 r 2 − 4 G 2 m u 2 (39)</p><p>We can decompose the age of the universe Δt<sub>u</sub> into two parts, Δt<sub>hu</sub> and Δt<sub>0h</sub>. The value Δt<sub>hu</sub> represents the time elapsed between r = r<sub>h</sub> (at the horizon) and our actual position r = r<sub>u</sub> in the universe. The value Δt<sub>0h</sub> gives the time elapsed between r = 0 (at the Big Bang) and r = r<sub>h</sub> (at the horizon).</p><p>Δ t u = Δ t h u + Δ t 0 h ≈ ( 9.50 + 10.47 i ) &#215; 10 9     yearswhere     i = − 1 (40)</p><p>The imaginary time Δt<sub>0h</sub> means that it elapses independently of our time. We cannot see an event between r = 0 and r = r<sub>h</sub>, and an observer located between r = 0 and r<sub>h</sub> could not see us. The Δt<sub>hu</sub> equation is:</p><p>Δ t h u = 1 H 0 ( ( ω + 2 ln [ ω + β ( 2 + 5 ) ] − ln ( 4 ) ) 2 22 + 10 5 ) ≈ 7 10 H 0 where ω = β 2 ( 9 + 4 5 ) − 4 (41)</p><p>The precise equation for Δt<sub>0h</sub> is:</p><p>Δ t 0 h = − ( 2 + π ) H 0 22 + 10 5 i ≈ − 77 100 H 0 i (42)</p><p>The modulus of the complex age Δt<sub>u</sub> gives the universe’s apparent age T<sub>u</sub>.</p><p>T u = | Δ t u | = | Δ h u + Δ t 0 h | = ( Δ t h u ) 2 + ( Δ t 0 h i ) 2 ≈ 14.14 &#215; 10 9     years (43)</p><p>T u = 1 H 0 ( ( ω + 2 ln [ ω + β ( 2 + 5 ) ] − ln ( 4 ) ) 2 22 + 10 5 ) 2 + ( [ − ( 2 + π ) 22 + 10 5 ] i ) 2 ︸ η ≈ 1 ( withabout4 .25%oferror ) (44)</p><p>As the square root over the accolade is approximatively equal to 1, we get:</p><p>T u ≈ 1 H 0 ≈ 13.56 &#215; 10 9     years (45)</p><p>The value of the correction factor between Equations (43) and (45) is η.</p><p>η = H 0 T u = H 0 ( Δ t h u ) 2 + ( Δ t 0 h i ) 2 ≈ 1.042516951 (46)</p><p>This η explains why scientists currently measure two values of H<sub>0</sub>. Scientists can only size the apparent age of the universe with different techniques. They cannot measure the real part and the imaginary part of the universe’s age.</p><p>There is no “local” or “far” value of H<sub>0</sub>. There is only one H<sub>0</sub>. Some techniques give H<sub>0</sub> directly, and others need a correction factor. There is no need for any correction factor when H<sub>0</sub> is calculated from Equation (33), measured with the CMB temperature with Equation (16), or with the universal gravitational constant G with Equation (34). Other techniques may get similar results than Equation (43), and if we impose that value to fit with Equation (45), we get H ′ 0 .</p><p>H ′ 0 = 1 | Δ t u | ≈ 1 14.14 &#215; 10 9     years ≈ H 0 η ≈ 69.2 km ⋅ s − 1 ⋅ MParsec − 1 (47)</p><p>However, Equation (45) gives the actual H<sub>0</sub> value:</p><p>H 0 ≈ 1 13.56 &#215; 10 9     years ≈ 72.1 km ⋅ s − 1 ⋅ MParsec − 1 (48)</p><p>If scientists could measure the real part of the universe’s age and associate this value with 1/H<sub>0</sub>, they would obtain the following value.</p><p>H 0 ≈ 1 9.50 &#215; 10 9     years ≈ 102.94 km ⋅ s − 1 ⋅ MParsec − 1 (49)</p><p>If scientists could measure the imaginary part somehow, the association of this value with 1/H<sub>0</sub> (like in Equation (45)) would give the following H<sub>0</sub> value.</p><p>H 0 ≈ 1 10.47 &#215; 10 9     years ≈ 93.39 km ⋅ s − 1 ⋅ MParsec − 1 (50)</p><p>with different types of experiments to measure the apparent age of the universe, scientists usually get either ~H<sub>0</sub> ≈ 69.2 or ~72.1 km·s<sup>−1</sup>·Mparsec<sup>−1</sup>. We assume that all calibration factors are used. New techniques could require other unknown corrective factors that have nothing to do with the related phenomenon.</p><p>The articles rarely give enough details to check if the process used needs η. Scientists must verify if the η factor is required for their approach.</p></sec><sec id="s5"><title>5. Other Experimental Measurements of Hubble Constant H<sub>0</sub></title><p>In 1929, Hubble made the first observational-based measurements with cepheids and got H<sub>0</sub> ≈ 500 km·s<sup>−1</sup>·MParsec<sup>−1</sup> [<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]. Sadly, even with a correct principle, his value is higher than the typical value due to errors in distance calibrations.</p><p>Let us validate our theoretical H<sub>0</sub> with an adequate interpretation of 508 measurements found on the Internet. The ends of their tolerance ranges give 1016 values. To find H<sub>0</sub> that has the highest probability to be measured, we compile the number of crossings with the tolerance ranges for each value of H<sub>0</sub>. It generates a curve with two tips (<xref ref-type="fig" rid="fig1">Figure 1</xref>). The higher it is, the greater the chances are that this value of H<sub>0</sub> may be part of many tolerance ranges among the collected data.</p><p>A simple statistical phenomenon may be described with a Gaussian function. For fitting a wavy curve, it is necessary to make the sum of many Gaussians. A simpler model with fewer degrees of liberty must always be privileged.</p><p>A curve fit is done by summing different Gaussians (shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>). A better gap fitting reduces the risk of finding other results. Thus, we gave a heavier weight (&#215;10) to all data located between 69.2 and 72.1 km·s<sup>−1</sup>·MParsec<sup>−1</sup> (from our theory). We tried with and without this approach, and it gives about the same result. As it improves the gap fitting, we kept this approach.</p><p>Each tip in <xref ref-type="fig" rid="fig1">Figure 1</xref> is approximated in <xref ref-type="fig" rid="fig2">Figure 2</xref> with two positive Gaussians. We force these curves to be around two means, even though there are four positive curves. It removes two degrees of liberty. We must add a negative Gaussian to model the gap between the two mean values. We must elaborate on this negative Gaussian. Our theory predicts “two close values” of H<sub>0</sub>. On the curve, a deep gap shows up. It is impossible to get such a gap by only adding positives Gaussians which give two little bumps without any gap. To get a real gap, we must add a negative Gaussian. Let us see in <xref ref-type="fig" rid="fig3">Figure 3</xref> what would look like a curve fit without any negative Gaussian. Since the tips are close, they mix up to build only one tip.</p><p>The Gaussian sum in <xref ref-type="fig" rid="fig3">Figure 3</xref> peaks around H<sub>0</sub> ≈ 71.11 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. The result is not close to our theoretical H<sub>0</sub> ≈ 72.09548580 km·s<sup>−1</sup>·MParsec<sup>−1</sup> (Equation (33)), but it is about what is found if statistics were used through the whole data set, thinking they should see only one tip. Moreover, Jang &amp; Lee showed a similar value of H<sub>0</sub> ≈ 71.17 km·s<sup>−1</sup>·MParsec<sup>−1</sup> (listed in our software in Annex A) that supposedly reduces the tension between the values obtained by cepheids (calibrated on SNe Ia) and CMB.</p><p>In <xref ref-type="fig" rid="fig1">Figure 1</xref>, we find two groups around H<sub>0</sub> ≈ 69.7 and 71.8 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. It is known that there is currently a tension between two groups [<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>]. A significant gap appears between the two tips. The only way to create such a gap is to</p><p>withdraw values nearby a specific value. It would then create a negative Gaussian, such as in <xref ref-type="fig" rid="fig2">Figure 2</xref>. It is delicate to debate why some values may have been withdrawn. It could be intentional or not. In the past, it was difficult to see a difference between these groups. Now, the tolerances are small enough to clearly see two groups. With recent growing tensions between these two clans, some may be inclined to shrink or shift some tolerance ranges when it overlaps with neighbor values.</p><p>In <xref ref-type="fig" rid="fig4">Figure 4</xref>, we apply η to the curves around H<sub>0</sub> ≈ 69.882 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. Then, all curves stand around H<sub>0</sub> ≈ 72.36 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. Then, with the curves of <xref ref-type="fig" rid="fig4">Figure 4</xref>, we build the curve in <xref ref-type="fig" rid="fig5">Figure 5</xref>. <xref ref-type="fig" rid="fig6">Figure 6</xref> is a zoom of its tip.</p><p>We want to know the precise value of H<sub>0</sub> for which the derivative of the Gaussian summation is 0. It corresponds to the highest probability of getting the true H<sub>0</sub> value. Unfortunately, the derivative of a Gaussian summation is not an easy equation to get in a software. We rather use a numerical technic to get it. In <xref ref-type="fig" rid="fig6">Figure 6</xref>, we show a zoom of the quadratic curve fit around the tip value. Using the equation, we take the derivative and find its maximum. The quadratic equation has the following form:</p><p>y ( x ) = A x 2 + B x + C Atthetip,theslopeis : y ′ ( x ) = d x d y = 2 A x + B = 0 → x = − B 2 A where x = H 0 , y = numberofcrossingswithdifferenttoleranceranges (51)</p><p>H 0 = − B 2 A ≈ 2423.2459592464 2 &#215; 16.8057572117 ≈ 72.0957088907   km ⋅ s − 1 ⋅ MParsec − 1 (52)</p><p>This result is well centered on our theoretical value within 3 parts per million. Our approach considers that both clans are someway right. Indeed, their different approaches and results also highlight a new phenomenon. It gives credit to our theory of the universe’s complex age that predicts a few possible fake H<sub>0</sub> values.</p><p>We have 508 data. Each has a tolerance range (that may be symmetrical or not) that generates two H<sub>0</sub> values. Therefore, there are a total of i<sub>max</sub> = 1016 data at the end. The following equation depicts the statistical error e<sub>t</sub>:</p><p>e t ≈ ∑ i = 1 i = i max e i 2 i max (53)</p><p>We mention that 16 H<sub>0</sub> values in our software in Annex A come from statistics. We kept them since some are mixed up with new valuable data information. So, we modify Equation (53) to remove them to reduce their impact on the total e<sub>t</sub> error. We use the following equation where n = 2 &#215; 16 = 32 (each data generates two H<sub>0</sub> values) is the number of elements to exclude from our sample. The total e<sub>t</sub> error reduces with the square root of the number of elements included in our sample.</p><p>e t ≈ ∑ i = 1 i = i max e i 2 i max ⋅ [ i max i max − n ] (54)</p><p>If n = 0, we fall back on Equation (53). With i<sub>max</sub> = 1016, Equation (53) gives e<sub>t</sub> ≈ &#177;0.32 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. With i<sub>max</sub> = 1016 and n = 32, Equation (54) rounds up to e<sub>t</sub> &#177; 0.33 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. The impact of these n elements has a very little impact.</p><p>H 0 ≈ 72.0957 &#177; 0.33   km ⋅ s − 1 ⋅ MParsec − 1 (55)</p><p>In Annex A, we supply the software used to get this result. All the main steps enumerated in this article are clearly shown. The software uses starting values (found via Excel) to fit the original curve with 5 Gaussian curves (#0 to #4 to use the same numbers as the software). Each Gaussian uses three parameters: μ is the mean value, σ represents the variance, and m is a multiplication factor.</p><p>f ( H 0 ) ≈ m σ 2 π e − 1 2 ( H 0 − μ σ ) 2 (56)</p><p>Here are the values for the 5 Gaussian curves used to fit the original curve:</p><disp-formula id="scirp.112694-formula3"><label>(57)</label><graphic position="anchor" xlink:href="//html.scirp.org/file/4-7504522x92.png?20220211163745470"  xlink:type="simple"/></disp-formula><p>For Gaussians #1 and #2, we force the software to use the same mean value. We do the same thing for Gaussians #3 and #4. We also note that the multiplication factor m of Gaussian #0 is negative. With these values, we stopped iterating when the sum of squares of errors was lower than 22000. We see in <xref ref-type="fig" rid="fig1">Figure 1</xref> that the obtained approximated curve fits well the original curve. In our software (Annex A), the iterations start with values close to what they should be.</p><p>The specificity of our approach is to say that the two clans are someway right. However, we must apply a correction factor to one of them. Indirectly, it gives credit to a complex universe age that predicts a few possible fake values of H<sub>0</sub>.</p><p>After reading this article, scientists should continue their work as they were doing, without applying any correction factor to their raw data. The correction factor should only be used on the final Gaussian curve to analyze data.</p></sec><sec id="s6"><title>6. A Reminder of Different Useful Identities</title><p>To avoid repeating everything unnecessarily, we recall different identities that will be used later to determine H<sub>0</sub>. Planck units are commonly defined as follows.</p><p>Planckmass : m p = h c 2 π G ≈ 2.18 &#215; 10 − 8     kg (58)</p><p>Plancktime : t p = h G 2 π c 5 = L p c ≈ 5.91 &#215; 10 − 44     s (59)</p><p>Plancklength : L p = h G 2 π c 3 = c t p ≈ 1.61 &#215; 10 − 35     m (60)</p><p>PlanckTemperature : T p = h c 3 2 π G k b 2 = m p c 2 k b ≈ 1.42 &#215; 10 32     K (61)</p><p>Planckcharge : q p = 2 c h ε 0 = − q e α ≈ 1.88 &#215; 10 − 18     C (62)</p><p>The fine-structure constant α is linked to Rydberg constant R<sub>∞</sub> and the electron mass m<sub>e</sub> by the following equation:</p><p>R ∞ = c m e α 2 2 h (63)</p><p>The speed of light c is given as a function of μ<sub>0</sub> and ε<sub>0</sub>.</p><p>c = 1 μ 0 ε 0 (64)</p><p>Associating the mass-energy of a Planck particle with its wave energy and then, using Equations (31), (32), (64), and (62), we get Planck charge q<sub>p</sub> defined several ways and as a function of c, G, and h like the other Planck units.</p><p>q p = 2 h c μ 0 = 4 π m p L p μ 0 = β G h 2 π μ 0 r e 2 c 4 α 19 (65)</p><p>The electron’s charge is determined from the mass of the electron m<sub>e</sub>, the classical electron radius r<sub>e</sub>, and the vacuum permeability μ<sub>0</sub>.</p><p>q e = 4 π m e r e μ 0 ≈ − 1.60 &#215; 10 − 19     C (66)</p><p>Let us calculate the precise value of the average temperature T of the CMB. We first make equal Equations (16) and (33). Then, we replace G by Equation (31), and we get rid of Planck constant h by its value from Equation (32).</p><p>T = m e c 2 k b ( 15 β 6 α 17 π 3 ) 1 / 4 ≈ 2.7367958 ( 16 )   K (67)</p><p>This CMB temperature is like Kimura with 2.737 K [<xref ref-type="bibr" rid="scirp.112694-ref23">23</xref>].</p></sec><sec id="s7"><title>7. Different Equations to Calculate H<sub>0</sub></title><p>For an academic purpose and to show the interdependence of H<sub>0</sub> with the other “constants”, we will enumerate equations using various universe parameters. Some overcome the inherent difficulties in measuring H<sub>0</sub> and show a roundabout way of obtaining an accurate value of it. We also find some others which depend on interesting values, or more precise ones. Using the constants c, k<sub>b</sub>, T, m<sub>e</sub>, r<sub>e</sub>, h, G, μ<sub>0</sub>, ε<sub>0</sub>, m<sub>u</sub>, R<sub>u</sub>, R<sub>∞</sub>, q<sub>e</sub>, q<sub>p</sub>, t<sub>p</sub>, l<sub>p</sub>, T<sub>p</sub>, m<sub>p</sub>, m<sub>ph</sub>, and β , we find many equations.</p><p>The H<sub>0</sub> parameter is not constant since 1/H<sub>0</sub> represents an approximation of the apparent universe’s age, and H<sub>0</sub> get smaller over time. Since the universe is old, H<sub>0</sub> changes slowly. If the constancy of all the universe’s parameters is maintained as it is currently done in metrology, the universe’s age and H<sub>0</sub> will seem constant.</p><p>Results of 508 different experiences reduce the error by 508<sup>1/2</sup> ≈ 22.5. It may look like a significant number, but it is nothing besides what has been done to measure the electron characteristics accurately. Particle accelerators use millions of electrons at each experiment, and they repeat these many times to find something new. Computers analyze the collisions’ results to make the electron’s characteristics more and more accurate. It is why there is no manner to get better results than that of Equation (33), as it is based on well-known characteristics of the electron. We will see further many other equations that give precise results.</p><p>Replacing G by Equation (31) in Equation (16), we get Equation (68).</p><p>H 0 = π 3 k b 2 T 2 α 9 8 r e 15 m e c 3 h 3 β 5 (68)</p><p>Replacing h in Equation (68) by using Equation (32), we get Equation (69).</p><p>H 0 = k b 2 T 2 π 3 α 21 15 r e 2 m e 4 β 5 c 6 (69)</p><p>Replacing h in Equation (16) by using Equation (32), we get Equation (70).</p><p>H 0 = k b 2 T 2 β 2 π 3 G α 15 r e 3 m e 3 c 8 (70)</p><p>Replacing T in Equation (70) by using Equation (67), we get Equation (71).</p><p>H 0 = β α 9 G m e r e 3 (71)</p><p>Using Equation (32) in Equation (33), we get Equation (72).</p><p>H 0 = 2 π m e c 2 α 18 β h (72)</p><p>With Equations (63) and (72), we get the most accurate equation.</p><p>H 0 = 4 π c R ∞ α 16 β (73)</p><p>Using Equation (31) in Equation (73), we get Equation (74).</p><p>H 0 = 4 π G m e R ∞ β 3 / 2 c r e α 4 (74)</p><p>Equation (74) gives H<sub>0</sub> with G<sub>2014</sub> (from CODATA 2014). The measurement of H<sub>0</sub>(G<sub>2014</sub>) ≈ 72.105(36) km·s<sup>−1</sup>·MParsec<sup>−1</sup> is our fourth way to measure H<sub>0</sub>.</p><p>Using Equation (63) in Equation (74), we get Equation (75). This equation is also a good candidate for measuring H<sub>0</sub> as a function of G.</p><p>H 0 = 8 π G h R ∞ 2 β 3 / 2 r e c 2 α 4 (75)</p><p>Using Equation (32) in Equation (75), we get Equation (76).</p><p>H 0 = 16 π 2 G m e R ∞ 2 β 3 / 2 c α 7 (76)</p><p>This equation is another good candidate for measuring H<sub>0</sub> as a function of G. The measure still gives the same result as Equation (74).</p><p>We will enumerate other equations without making all the rather fastidious demonstrations. However, all these may be found from previous equations.</p><p>H 0 = 2 π m p h c 2 h (77)</p><p>H 0 = 2 c 2 π R ∞ α 55 G m e (78)</p><p>H 0 = β α 9 m e c r e 3 (79)</p><p>H 0 = 8 β G m e ( π R ∞ ) 3 α 9 (80)</p><p>H 0 = 8 c β r e ( π R ∞ ) 3 α 29 (81)</p><p>H 0 = 2 π c 5 α 57 h G (82)</p><p>H 0 = 2 c π β R ∞ α 25 r e (83)</p><p>H 0 = 2 π β m e c 3 α 37 h r e (84)</p><p>H 0 = 2 π 2 h ( k b 4 T 4 15 m u α 2 c 2 β 4 ) 1 / 3 (85)</p><p>H 0 = 2 π k b T p h α 57 (86)</p><p>H 0 = c μ 0 q e 2 α 19 β 4 π m e r e 2 (87)</p><p>H 0 = q e 2 α 19 β 4 π c ε 0 m e r e 2 (88)</p><p>H 0 = q p 2 α 18 β 2 h ε 0 r e (89)</p><p>H 0 = c μ 0 q p 2 α 20 β 4 π m e r e 2 (90)</p><p>H 0 = q p 2 α 20 β 4 π c ε 0 m e r e 2 (91)</p><p>H 0 = c β q p 2 α 19 4 π ε 0 k b T p r e 2 (92)</p><p>H 0 = c β q e 2 α 17 4 π ε 0 k b T p r e 2 (93)</p><p>H 0 = c q e 2 β 2 4 ε 0 k b T r e 2 ( 15 α 97 π 7 ) 1 / 4 (94)</p><p>H 0 = 2 k b T β h ( π 7 α 55 15 ) 1 / 4 (95)</p><p>H 0 = k b T β r e m e c ( π 3 α 59 15 ) 1 / 4 (96)</p><p>H 0 = 4 π k b T β c μ 0 q e 2 ( π 3 α 59 15 ) 1 / 4 (97)</p><p>H 0 = 4 π k b T β c μ 0 q p 2 ( π 3 α 55 15 ) 1 / 4 (98)</p><p>H 0 = G k b T c 3 r e 2 ( π 3 15 α 21 ) 1 / 4 (99)</p><p>H 0 = 2 G m e k b T h r e c 2 ( π 7 15 α 25 ) 1 / 4 (100)</p><p>H 0 = G m p k b T m e c 3 r e 2 ( π 3 α 21 15 β 2 ) 1 / 4 (101)</p><p>H 0 = G m u k b T m e c 3 r e 2 ( π 3 α 135 15 β 2 ) 1 / 4 (102)</p><p>H 0 = G m e k b T m p c 3 r e 2 ( π 3 β 2 15 α 63 ) 1 / 4 (103)</p><p>H 0 = 16 c G k b T ε 0 m e 2 q e 4 ( π 11 15 α 21 ) 1 / 4 (104)</p><p>H 0 = β m e 2 8 π 3 G c 3 α 15 h 3 (105)</p><p>H 0 = c 3 α 39 G m e β (106)</p><p>The last equation measures H<sub>0</sub> from G since all other constants are accurate. Many equations are excellent candidates for measuring H<sub>0</sub> as a function of G or T. These equations could represent valuable tools for cosmologists.</p><p>This document gives 42 equations of H<sub>0</sub> as a function of various universe parameters. Since H<sub>0</sub> may be defined using different parameters, we suggest that some of the most critical universe parameters are well linked, as much in the infinitely small as in the infinitely large, and H<sub>0</sub> is part of these.</p></sec><sec id="s8"><title>8. Why Is H<sub>0</sub> Not Really a Constant?</title><p>We want to explain why Hubble parameter H<sub>0</sub> cannot be constant over time. As simple as it is, the reverse of Hubble parameter H<sub>0</sub> is related to the apparent age of the universe (see Equation (45)). Consequently, the H<sub>0</sub> parameter is changing over time. It is, therefore, by abuse of language that we call H<sub>0</sub> the Hubble “constant”. To be more precise, we should say the Hubble “parameter”.</p><p>When H<sub>0</sub> is expressed in km·s<sup>−1</sup>·MParsec<sup>−1</sup>, the ninth digit after the dot changes every year. It goes completely unnoticed. More than that, even if we could achieve this precision in our measurements of H<sub>0</sub>, it would still go unnoticed since we forced c to be constant in 1983. In metrology, scientists choose the speed of light as a standard. Even though c changes every year, if we force it to be constant, we willfully readjust all other constants and units (distance, time, and mass) as a function of c to keep it constant. Then, H<sub>0</sub> looks constant as other parameters.</p></sec><sec id="s9"><title>9. Conclusions</title><p>This article aimed to show that our theoretical value from Equation (33) (giving H<sub>0</sub> ≈ 72.09548580(32) km·s<sup>−1</sup>·MParsec<sup>−1</sup>) [<xref ref-type="bibr" rid="scirp.112694-ref6">6</xref>] is the right one, despite a growing tension [<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>] between values around 69.2 and 72.1 km·s<sup>−1</sup>·MParsec<sup>−1</sup>.</p><p>With 508 data (from [<xref ref-type="bibr" rid="scirp.112694-ref24">24</xref>] to [<xref ref-type="bibr" rid="scirp.112694-ref310">310</xref>] shown in our software in Annex A), a graph showing the actual tension [<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>] between two values is shown. We decomposed the curve into Gaussians. A negative one is required to explain the large gap between the two H<sub>0</sub> values, and it is due to withdrawn values. So, we restored them by removing that curve. Then, we applied a η ≈ 1.042516951 correction factor (from our theory) to the curves located at ~H<sub>0</sub> ≈ 69.2 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. Our theory highlights a misunderstanding of the link between 1/H<sub>0</sub> and the universe’s apparent age. With the proper correction factor applied, we get a statistical value of H<sub>0</sub> ≈ 72.0957 &#177; 0.33 km·s<sup>−1</sup>·MParsec<sup>−1</sup>, which is close to our theoretical value. Our discovery of the η factor may help to reduce the tension between scientists. Someway we show that even if two H<sub>0</sub> values seem to be commonly found with various techniques, both are accurate if a proper correction factor is used.</p><p>With a new cosmological model, we get an apparent age of the universe of about 14.14 billion years. The exact formula is approximated from an elaborate integral result by the well-known 1/H<sub>0</sub> equation that gives 13.56 billion years. Different techniques may lead to either value. It depends if it is an attempt to measure the universe’s age locally or far away. There is no “local” or “distant” value of H<sub>0</sub>, as some may pretend [<xref ref-type="bibr" rid="scirp.112694-ref46">46</xref>] [<xref ref-type="bibr" rid="scirp.112694-ref47">47</xref>]. Sticking their measurement of the apparent age of the universe to 1/H<sub>0</sub>, most cosmologists get results that stand around 69.2 or 72.1 km·s<sup>−1</sup>·MParsec<sup>−1</sup>. Our hypothesis may explain the actual tension [<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>] relative to these two values. However, there is only one true H<sub>0</sub> value, and the other one is just misinterpreted as being the Hubble constant without quite being so.</p><p>Even if many theoretical equations of H<sub>0</sub> are shown in this article, we highlight that we also found a few interesting ways to measure the H<sub>0</sub> accurately using the CMB temperature T and the value of the universal gravitational constant G from CODATA 2014. These results confirm our theoretical value.</p><p>H<sub>0</sub> ≈ 72.06(90) km·s<sup>−1</sup>·MParsec<sup>−1</sup> and 71.95(50) km·s<sup>−1</sup>·MParsec<sup>−1</sup> from T,</p><p>H<sub>0</sub> ≈ 72.086(36) km·s<sup>−1</sup>·MParsec<sup>−1</sup> and 72.105(36) km·s<sup>−1</sup>·MParsec<sup>−1</sup> from G.</p><p>For an academic purpose, we enumerated 42 equations of H<sub>0</sub> using different parameters. These equations showed that H<sub>0</sub> is intricated with all other “constants”. For metrology purposes, the speed of light in a vacuum is forced to be constant to be an unchanging standard. If this situation is considered valid in a metrology context, H<sub>0</sub> should also be considered constant and become part of the CODATA. However, if 1/H<sub>0</sub> represents an approximation of the universe’s age, it would also make sense to say that H<sub>0</sub> is changing over time.</p><p>Einstein’s and Schwarzschild’s equations show that massive objects such as the universe influence the speed of light. As the universe expands, its density diminishes, and the local speed of light increases over time.</p><p>The fine-structure constant α is unitless and may be described as a ratio where the variation rate at the numerator counterbalances the variation rate at the denominator. Apart from α and β , all “constants” used to describe H<sub>0</sub> in our equations somehow emanate from fundamental units such as the meter, the second, and the kilogram. These units are now defined by the speed of light. As H<sub>0</sub> describes the universe’s age and depends on many unit-dependent “constants” based on c, we should consider c and all universe’s unit-dependent parameters as changing over time. Forcing c to be constant is necessary for metrology purposes, but it is not in the interest of physicists for explaining phenomena. An accurate value of H<sub>0</sub> has a great interest in deepening our understanding of the universe.</p></sec><sec id="s10"><title>Conflicts of Interest</title><p>The author claims that he has no conflict of interest in connection with the publication of this article.</p></sec><sec id="s11"><title>Cite this paper</title><p>Mercier, C. (2021) A New Physics Would Explain What Looks Like an Irreconcilable Tension between the Values of Hubble Constants and Allows H<sub>0</sub> to Be Calculated Theoretically Several Ways. Journal of Modern Physics, 12, 1656-1707. https://doi.org/10.4236/jmp.2021.1212098</p></sec><sec id="s12"><title>Annex A (C++ Software)</title><p>// This software finds &quot;the best&quot; experimental value of H0 with a set of 508 data</p><p>//Compiled on Dev-C++ 5.11 available for free at:</p><p>// https://sourceforge.net/projects/orwelldevcpp/</p><p>#include</p><p>#include</p><p>#include</p><p>#define printf __mingw_printf</p><p>#define nbH0 508 //Number of measurements of H0 analyzed</p><p>#define Pi 3.141592654 //Definition of Pi</p><p>double Mean[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>],Sigma[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>],Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>];//Caracteristics of Gaussian curves</p><p>double A,B,C; //Coefficients of the quadratic equation of the tip</p><p>double LMSTip; //Least mean square for the approximation tip curve</p><p>double BEH; //Best estimate of H0</p><p>double H0[2*nbH0-1],NbCrossings[2*nbH0-1];</p><p>double nbCrossings[2*nbH0-1]; //Vector of number of crossings</p><p>double Accuracy_ppm; //Accuracy of H0 compared to the theoretical value</p><p>double TVH = 72.09548580; //Theoretical value of H0 (in km/(s*MParsec)</p><p>unsigned int PosTipIndex; //Index corresponding to the tip of nbCrossings array</p><p>int n = 20; //Sample before &amp; after PosTipIndex to build the tip equation</p><p>double Sqr(double value) {return value*value;} //***Returns the square value</p><p>//***Function that returns the square root value</p><p>double Sqrt(double Value) {</p><p>double D; /*Dummy value*/ double V; /*Returned value*/ int i; /*Counter*/</p><p>V=0; D=Value;</p><p>for (i=0;i&lt;=50;i++) { //Gives 50 bits of precision</p><p>D=-D/2;</p><p>if (D&lt;0) while (V*V&gt;Value) V=V+D; else while (V*V</p><p>return V;</p><p>} //End of Sqrt</p><p>double Exp(double Value) { return pow(2.718281828,Value);} //***e^Value</p><p>//***This procedure creates a table of 2*nbH increasing values</p><p>//***of H0[i] with the tolerances T[i] and the signs +/- Variation[i].</p><p>void CreateTableOfCrossingH0Ranges(void) {</p><p>double PT[nbH0],NT[nbH0]; //Positive tolerance and negative tolerance</p><p>double Variation[2*nbH0]; //Variation from the tolerance range</p><p>double DH0,DSgn; //Dummy H0 and Sgn used to put H in increasing order</p><p>int DeltaCrossings; //Variation of on the number of crossings</p><p>int i,j,k; //Counters</p><p>i=0;</p><p>//We enumerate all H0 values and their tolerance range found on Internet</p><p>//In brackets, we add the bibliographic references</p><p>H0[i]=69; PT[i]=+16; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref24">24</xref>] Abbott et al.</p><p>H0[i]=70; PT[i]=+2.7; NT[i++]=-2.7; // [<xref ref-type="bibr" rid="scirp.112694-ref25">25</xref>] Addisson</p><p>H0[i]=72.4; PT[i]=+3.9; NT[i++]=-4.8; // [<xref ref-type="bibr" rid="scirp.112694-ref25">25</xref>] Addisson</p><p>H0[i]=73.1; PT[i]=+3.3; NT[i++]=-3.9; // [<xref ref-type="bibr" rid="scirp.112694-ref25">25</xref>] Addisson</p><p>H0[i]=73.2; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref25">25</xref>] Addisson</p><p>H0[i]=68.7; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref25">25</xref>] Addisson</p><p>H0[i]=73.5; PT[i]=+5.3; NT[i++]=-5.3; // [<xref ref-type="bibr" rid="scirp.112694-ref26">26</xref>] Baxter &amp; Sherwin</p><p>H0[i]=73.3; PT[i]=+0.7; NT[i++]=-0.7; // [<xref ref-type="bibr" rid="scirp.112694-ref27">27</xref>] Blakeslee et al.</p><p>H0[i]=73.78; PT[i]=+0.84; NT[i++]=-0.84; // [<xref ref-type="bibr" rid="scirp.112694-ref28">28</xref>] Bonilla</p><p>H0[i]=73.577; PT[i]=+0.106; NT[i++]=-0.106; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.493; PT[i]=+0.144; NT[i++]=-0.144; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.222; PT[i]=+0.262; NT[i++]=-0.262; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.664; PT[i]=+0.223; NT[i++]=-0.223; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.576; PT[i]=+0.105; NT[i++]=-0.105; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.513; PT[i]=+0.142; NT[i++]=-0.142; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.192; PT[i]=+0.265; NT[i++]=-0.265; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=73.678; PT[i]=+0.223; NT[i++]=-0.223; // [<xref ref-type="bibr" rid="scirp.112694-ref29">29</xref>] Dainotti et al.</p><p>H0[i]=71.8; PT[i]=+3.9; NT[i++]=-3.3; // [<xref ref-type="bibr" rid="scirp.112694-ref30">30</xref>] Denzel et al.</p><p>H0[i]=72.94; PT[i]=+0.75; NT[i++]=-0.75; // [<xref ref-type="bibr" rid="scirp.112694-ref31">31</xref>] Di Valentino</p><p>H0[i]=72.7; PT[i]=+1.1; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref31">31</xref>] Di Valentino</p><p>H0[i]=68.8; PT[i]=+45.7; NT[i++]=-25.5; // [<xref ref-type="bibr" rid="scirp.112694-ref32">32</xref>] Gayathri et al.</p><p>H0[i]=62.3; PT[i]=+9.1; NT[i++]=-9.1; // [<xref ref-type="bibr" rid="scirp.112694-ref33">33</xref>] Hagstotz et al.</p><p>H0[i]=70.5; PT[i]=+2.37; NT[i++]=-2.37; // [<xref ref-type="bibr" rid="scirp.112694-ref34">34</xref>] Kethan et al.</p><p>H0[i]=72.86; PT[i]=+0.036; NT[i++]=-0.036; //Mercier (this document)</p><p>H0[i]=72.105; PT[i]=+0.036; NT[i++]=-0.036; //Mercier (this document)</p><p>H0[i]=68.3; PT[i]=+4.6; NT[i++]=-4.6; // [<xref ref-type="bibr" rid="scirp.112694-ref35">35</xref>] Mukherjee et al.</p><p>H0[i]=70; PT[i]=+0.5; NT[i++]=-0.5; // [<xref ref-type="bibr" rid="scirp.112694-ref36">36</xref>] Park et al.</p><p>H0[i]=65.1; PT[i]=+3; NT[i++]=-5.4; // [<xref ref-type="bibr" rid="scirp.112694-ref37">37</xref>] Philcox et al.</p><p>H0[i]=65.6; PT[i]=+3.4; NT[i++]=-3.5; // [<xref ref-type="bibr" rid="scirp.112694-ref37">37</xref>] Philcox et al.</p><p>H0[i]=70.6; PT[i]=+3.7; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref37">37</xref>] Philcox et al.</p><p>H0[i]=78.3; PT[i]=+2.9; NT[i++]=-2.9; // [<xref ref-type="bibr" rid="scirp.112694-ref38">38</xref>] Qi et al.</p><p>H0[i]=73.6; PT[i]=+1.8; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref38">38</xref>] Qi et al.</p><p>H0[i]=73; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref39">39</xref>] Riess et al.</p><p>H0[i]=73.2; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref39">39</xref>] Riess et al.</p><p>H0[i]=72.1; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref40">40</xref>] Soltis et al.</p><p>H0[i]=69.5; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref41">41</xref>] Wang &amp; Giannios</p><p>H0[i]=71; PT[i]=+20; NT[i++]=-20; // [<xref ref-type="bibr" rid="scirp.112694-ref42">42</xref>] Zhang et al.</p><p>H0[i]=67.4; PT[i]=+0.5; NT[i++]=-0.5; // [<xref ref-type="bibr" rid="scirp.112694-ref43">43</xref>] Aghanim et al.</p><p>H0[i]=67.73; PT[i]=+0.41; NT[i++]=-0.41; // [<xref ref-type="bibr" rid="scirp.112694-ref44">44</xref>] Benevento</p><p>H0[i]=68.22; PT[i]=+0.39; NT[i++]=-0.39; // [<xref ref-type="bibr" rid="scirp.112694-ref44">44</xref>] Benevento</p><p>H0[i]=72.5; PT[i]=+1.85; NT[i++]=-1.85; // [<xref ref-type="bibr" rid="scirp.112694-ref44">44</xref>] Benevento</p><p>H0[i]=69.17; PT[i]=+1.09; NT[i++]=-1.09; // [<xref ref-type="bibr" rid="scirp.112694-ref44">44</xref>] Benevento</p><p>H0[i]=74.5; PT[i]=+5.6; NT[i++]=-6.1; // [<xref ref-type="bibr" rid="scirp.112694-ref45">45</xref>] Birrer et al.</p><p>H0[i]=67.4; PT[i]=+4.1; NT[i++]=-3.2; // [<xref ref-type="bibr" rid="scirp.112694-ref45">45</xref>] Birrer et al.</p><p>H0[i]=75.35; PT[i]=+1.68; NT[i++]=-1.68; // [<xref ref-type="bibr" rid="scirp.112694-ref46">46</xref>] Camarena &amp; Marra</p><p>H0[i]=74; PT[i]=+0.625; NT[i++]=-0.625; // [<xref ref-type="bibr" rid="scirp.112694-ref47">47</xref>] Chang &amp; Zhu</p><p>H0[i]=73.8; PT[i]=+6.3; NT[i++]=-5.8; // [<xref ref-type="bibr" rid="scirp.112694-ref48">48</xref>] Coughlin et al.</p><p>H0[i]=71.2; PT[i]=+3.2; NT[i++]=-3.1; // [<xref ref-type="bibr" rid="scirp.112694-ref48">48</xref>] Coughlin et al.</p><p>H0[i]=72.4; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref49">49</xref>] D'Agostino</p><p>H0[i]=71.5; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref49">49</xref>] D'Agostino</p><p>H0[i]=71.54; PT[i]=+1.78; NT[i++]=-1.78; // [<xref ref-type="bibr" rid="scirp.112694-ref50">50</xref>] Dai WM et al.</p><p>H0[i]=73.12; PT[i]=+1.14; NT[i++]=-1.14; // [<xref ref-type="bibr" rid="scirp.112694-ref50">50</xref>] Dai WM et al.</p><p>H0[i]=66.2; PT[i]=+4.4; NT[i++]=-4.2; // [<xref ref-type="bibr" rid="scirp.112694-ref51">51</xref>] Dietrich et al.</p><p>H0[i]=69.9; PT[i]=+0.84; NT[i++]=-0.86; // [<xref ref-type="bibr" rid="scirp.112694-ref52">52</xref>] Gonzalez et al.</p><p>H0[i]=71; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref53">53</xref>] Gonz&#225;lez-Serrena et al.</p><p>H0[i]=74.62; PT[i]=+12.35; NT[i++]=-11.34; // [<xref ref-type="bibr" rid="scirp.112694-ref54">54</xref>] Haboury</p><p>H0[i]=71.89; PT[i]=+11.02; NT[i++]=-10.17; // [<xref ref-type="bibr" rid="scirp.112694-ref54">54</xref>] Haboury</p><p>H0[i]=76.44; PT[i]=+55.76; NT[i++]=-50.17; // [<xref ref-type="bibr" rid="scirp.112694-ref54">54</xref>] Haboury</p><p>H0[i]=50.9; PT[i]=+31.1; NT[i++]=-31.9; // [<xref ref-type="bibr" rid="scirp.112694-ref54">54</xref>] Haboury</p><p>H0[i]=50.81; PT[i]=+28.19; NT[i++]=-27.81; // [<xref ref-type="bibr" rid="scirp.112694-ref54">54</xref>] Haboury</p><p>H0[i]=71; PT[i]=+2; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref55">55</xref>] Harvey</p><p>H0[i]=65.9; PT[i]=+1.5; NT[i++]=-1.5; // [<xref ref-type="bibr" rid="scirp.112694-ref56">56</xref>] Holanda et al.</p><p>H0[i]=65.9; PT[i]=+4.4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref56">56</xref>] Holanda et al.</p><p>H0[i]=64.3; PT[i]=+4.5; NT[i++]=-4.4; // [<xref ref-type="bibr" rid="scirp.112694-ref56">56</xref>] Holanda et al.</p><p>H0[i]=66.8; PT[i]=+13.4; NT[i++]=-9.2; // [<xref ref-type="bibr" rid="scirp.112694-ref57">57</xref>] Howlett &amp; Davis</p><p>H0[i]=64.8; PT[i]=+7.3; NT[i++]=-7.2; // [<xref ref-type="bibr" rid="scirp.112694-ref57">57</xref>] Howlett &amp; Davis</p><p>H0[i]=75.8; PT[i]=+5.2; NT[i++]=-4.9; // [<xref ref-type="bibr" rid="scirp.112694-ref58">58</xref>] Jaeger et al.</p><p>H0[i]=65.8; PT[i]=+3.5; NT[i++]=-3.5; // [<xref ref-type="bibr" rid="scirp.112694-ref59">59</xref>] Kim et al.</p><p>H0[i]=72.3; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref60">60</xref>] Kreisch et al.</p><p>H0[i]=71.5; PT[i]=+11.9; NT[i++]=-10.6; // [<xref ref-type="bibr" rid="scirp.112694-ref61">61</xref>] Li &amp; Zhang</p><p>H0[i]=74.7; PT[i]=+5.8; NT[i++]=-5.8; // [<xref ref-type="bibr" rid="scirp.112694-ref62">62</xref>] Lombriser</p><p>H0[i]=72.06; PT[i]=+0.09; NT[i++]=-0.09; // [<xref ref-type="bibr" rid="scirp.112694-ref7">7</xref>] Mercier</p><p>H0[i]=74; PT[i]=+1.6; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref63">63</xref>] Millon et al.</p><p>H0[i]=74.2; PT[i]=+1.7; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref63">63</xref>] Millon et al.</p><p>H0[i]=50.4; PT[i]=+28.1; NT[i++]=-19.5; // [<xref ref-type="bibr" rid="scirp.112694-ref64">64</xref>] Mukherjee et al.</p><p>H0[i]=62.2; PT[i]=+29.5; NT[i++]=-19.7; // [<xref ref-type="bibr" rid="scirp.112694-ref64">64</xref>] Mukherjee et al.</p><p>H0[i]=43.1; PT[i]=+24.6; NT[i++]=-11.4; // [<xref ref-type="bibr" rid="scirp.112694-ref64">64</xref>] Mukherjee et al.</p><p>H0[i]=67.6; PT[i]=+4.3; NT[i++]=-4.2; // [<xref ref-type="bibr" rid="scirp.112694-ref64">64</xref>] Mukherjee et al.</p><p>H0[i]=68.6; PT[i]=+14; NT[i++]=-8.5; // [<xref ref-type="bibr" rid="scirp.112694-ref65">65</xref>] Nicolaou et al.</p><p>H0[i]=69.6; PT[i]=+1; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref66">66</xref>] Niedermann and Sloth</p><p>H0[i]=71.4; PT[i]=+1; NT[i++]=-1; // [<xref ref-type="bibr" rid="scirp.112694-ref66">66</xref>] Niedermann and Sloth</p><p>H0[i]=72; PT[i]=+12; NT[i++]=-8.2; // [<xref ref-type="bibr" rid="scirp.112694-ref67">67</xref>] Palmese et al.</p><p>H0[i]=69.03; PT[i]=+0.87; NT[i++]=-0.87; // [<xref ref-type="bibr" rid="scirp.112694-ref68">68</xref>] Pandey et al.</p><p>H0[i]=70.6; PT[i]=+1.1; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref68">68</xref>] Pandey et al.</p><p>H0[i]=68.44; PT[i]=+0.52; NT[i++]=-0.52; // [<xref ref-type="bibr" rid="scirp.112694-ref68">68</xref>] Pandey et al.</p><p>H0[i]=68.1; PT[i]=+0.58; NT[i++]=-0.58; // [<xref ref-type="bibr" rid="scirp.112694-ref68">68</xref>] Pandey et al.</p><p>H0[i]=73.9; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref69">69</xref>] Pesce et al.</p><p>H0[i]=68.6; PT[i]=+1.8; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref70">70</xref>] Pogosian et al.</p><p>H0[i]=74.03; PT[i]=+1.42; NT[i++]=-1.42; // [<xref ref-type="bibr" rid="scirp.112694-ref71">71</xref>] Rui-Yun et al.</p><p>H0[i]=75.1; PT[i]=+2.3; NT[i++]=-2.3; // [<xref ref-type="bibr" rid="scirp.112694-ref72">72</xref>] Schombert et al.</p><p>H0[i]=74.2; PT[i]=+2.7; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref73">73</xref>] Shajib et al.</p><p>H0[i]=67.52; PT[i]=+0.96; NT[i++]=-0.95; // [<xref ref-type="bibr" rid="scirp.112694-ref74">74</xref>] Sharov &amp; Sinyakov</p><p>H0[i]=70.87; PT[i]=+1.63; NT[i++]=-1.62; // [<xref ref-type="bibr" rid="scirp.112694-ref74">74</xref>] Sharov &amp; Sinyakov</p><p>H0[i]=69; PT[i]=+29; NT[i++]=-14; // [<xref ref-type="bibr" rid="scirp.112694-ref75">75</xref>] Vasylyev &amp; Filippenko</p><p>H0[i]=67; PT[i]=+41; NT[i++]=-26; // [<xref ref-type="bibr" rid="scirp.112694-ref75">75</xref>] Vasylyev &amp; Filippenko</p><p>H0[i]=71; PT[i]=+34; NT[i++]=-30; // [<xref ref-type="bibr" rid="scirp.112694-ref75">75</xref>] Vasylyev &amp; Filippenko</p><p>H0[i]=70; PT[i]=+29; NT[i++]=-18; // [<xref ref-type="bibr" rid="scirp.112694-ref75">75</xref>] Vasylyev &amp; Filippenko</p><p>H0[i]=72.3; PT[i]=+2.9; NT[i++]=-2.8; // [<xref ref-type="bibr" rid="scirp.112694-ref76">76</xref>] Vogl</p><p>H0[i]=75.3; PT[i]=+3; NT[i++]=-2.9; // [<xref ref-type="bibr" rid="scirp.112694-ref77">77</xref>] Wei &amp; Melia</p><p>H0[i]=75.3; PT[i]=+1.9; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref77">77</xref>] Wei &amp; Melia</p><p>H0[i]=67.9; PT[i]=+1.1; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref78">78</xref>] Wu et al.</p><p>H0[i]=72; PT[i]=+2.1; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref78">78</xref>] Wu et al.</p><p>H0[i]=73.65; PT[i]=+1.95; NT[i++]=-2.26; // [<xref ref-type="bibr" rid="scirp.112694-ref79">79</xref>] Yang et al.</p><p>H0[i]=67.95; PT[i]=+0.78; NT[i++]=-1.03; // [<xref ref-type="bibr" rid="scirp.112694-ref80">80</xref>] Zhang &amp; Huang</p><p>H0[i]=69.81; PT[i]=+2.22; NT[i++]=-2.7; // [<xref ref-type="bibr" rid="scirp.112694-ref80">80</xref>] Zhang &amp; Huang</p><p>H0[i]=66.75; PT[i]=+3.42; NT[i++]=-4.23; // [<xref ref-type="bibr" rid="scirp.112694-ref80">80</xref>] Zhang &amp; Huang</p><p>H0[i]=70.75; PT[i]=+1.55; NT[i++]=-1.55; // [<xref ref-type="bibr" rid="scirp.112694-ref81">81</xref>] Agrawal</p><p>H0[i]=73.7; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref82">82</xref>] Anderson</p><p>H0[i]=72.5; PT[i]=+2.1; NT[i++]=-2.3; // [<xref ref-type="bibr" rid="scirp.112694-ref83">83</xref>] Birrer</p><p>H0[i]=67.4; PT[i]=+0.5; NT[i++]=-0.5; // [<xref ref-type="bibr" rid="scirp.112694-ref84">84</xref>] Chang et al.</p><p>H0[i]=82.8; PT[i]=+9.4; NT[i++]=-8.3; // [<xref ref-type="bibr" rid="scirp.112694-ref85">85</xref>] Chen et al.</p><p>H0[i]=70.1; PT[i]=+5.3; NT[i++]=-4.5; // [<xref ref-type="bibr" rid="scirp.112694-ref85">85</xref>] Chen et al.</p><p>H0[i]=77; PT[i]=+4; NT[i++]=-4.6; // [<xref ref-type="bibr" rid="scirp.112694-ref85">85</xref>] Chen et al.</p><p>H0[i]=75.6; PT[i]=+3.2; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref85">85</xref>] Chen et al.</p><p>H0[i]=76.8; PT[i]=+2.6; NT[i++]=-2.6; // [<xref ref-type="bibr" rid="scirp.112694-ref85">85</xref>] Chen et al.</p><p>H0[i]=75.7; PT[i]=+4.5; NT[i++]=-4.4; // [<xref ref-type="bibr" rid="scirp.112694-ref86">86</xref>] Collett</p><p>H0[i]=76.8; PT[i]=+4.2; NT[i++]=-3.8; // [<xref ref-type="bibr" rid="scirp.112694-ref86">86</xref>] Collett</p><p>H0[i]=74.2; PT[i]=+3; NT[i++]=-2.9; // [<xref ref-type="bibr" rid="scirp.112694-ref86">86</xref>] Collett</p><p>H0[i]=67.6; PT[i]=+1.1; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref87">87</xref>] Cuceu et al.</p><p>H0[i]=67.4; PT[i]=+6; NT[i++]=-6.2; // [<xref ref-type="bibr" rid="scirp.112694-ref88">88</xref>] Dom&#237;nguez</p><p>H0[i]=66.6; PT[i]=+1.6; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref88">88</xref>] Dom&#237;nguez</p><p>H0[i]=70.3; PT[i]=+1.36; NT[i++]=-1.35; // [<xref ref-type="bibr" rid="scirp.112694-ref89">89</xref>] Dutta et al.</p><p>H0[i]=77; PT[i]=+37; NT[i++]=-18; // [<xref ref-type="bibr" rid="scirp.112694-ref90">90</xref>] Fishbach et al.</p><p>H0[i]=76; PT[i]=+19; NT[i++]=-13; // [<xref ref-type="bibr" rid="scirp.112694-ref90">90</xref>] Fishbach et al.</p><p>H0[i]=69.8; PT[i]=+0.8; NT[i++]=-0.8; // [<xref ref-type="bibr" rid="scirp.112694-ref91">91</xref>] Freedman et al.</p><p>H0[i]=68.09; PT[i]=+0.45; NT[i++]=-0.45; // [<xref ref-type="bibr" rid="scirp.112694-ref92">92</xref>] Guo et al.</p><p>H0[i]=69.34; PT[i]=+0.93; NT[i++]=-0.93; // [<xref ref-type="bibr" rid="scirp.112694-ref92">92</xref>] Guo et al.</p><p>H0[i]=69.67; PT[i]=+0.95; NT[i++]=-0.94; // [<xref ref-type="bibr" rid="scirp.112694-ref92">92</xref>] Guo et al.</p><p>H0[i]=69.36; PT[i]=+0.82; NT[i++]=-0.82; // [<xref ref-type="bibr" rid="scirp.112694-ref92">92</xref>] Guo et al.</p><p>H0[i]=69.25; PT[i]=+0.99; NT[i++]=-0.99; // [<xref ref-type="bibr" rid="scirp.112694-ref92">92</xref>] Guo et al.</p><p>H0[i]=74; PT[i]=+16; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref93">93</xref>] Hotokezaka et al.</p><p>H0[i]=70.3; PT[i]=+5.3; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref93">93</xref>] Hotokesaka et al.</p><p>H0[i]=82.4; PT[i]=+8.4; NT[i++]=-8.3; // [<xref ref-type="bibr" rid="scirp.112694-ref94">94</xref>] Jee et al.</p><p>H0[i]=67; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref95">95</xref>] Kozmanyan et al.</p><p>H0[i]=72.2; PT[i]=+2.1; NT[i++]=-2.1; // [<xref ref-type="bibr" rid="scirp.112694-ref96">96</xref>] Liao et al.</p><p>H0[i]=73; PT[i]=+2.8; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref96">96</xref>] Liao et al.</p><p>H0[i]=67.8; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref97">97</xref>] MacAulay et al.</p><p>H0[i]=67.37; PT[i]=+0.62; NT[i++]=-0.62; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=68.8; PT[i]=+1.6; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=73.9; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=67.68; PT[i]=+0.46; NT[i++]=-0.46; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=68.4; PT[i]=+1; NT[i++]=-1; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=69.2; PT[i]=+1.5; NT[i++]=-1.5; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=67.51; PT[i]=+0.61; NT[i++]=-0.61; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=68.9; PT[i]=+1.1; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=72.1; PT[i]=+2.1; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=67.75; PT[i]=+0.46; NT[i++]=-0.46; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=68.59; PT[i]=+0.86; NT[i++]=-0.86; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=69.6; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref98">98</xref>] Martinelli</p><p>H0[i]=71.505; PT[i]=+0.03; NT[i++]=-0.03; // [<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>] Mercier</p><p>H0[i]=69; PT[i]=+1.7; NT[i++]=-1.7; // [<xref ref-type="bibr" rid="scirp.112694-ref99">99</xref>] Park &amp; Ratra</p><p>H0[i]=69.8; PT[i]=+1.8; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref99">99</xref>] Park &amp; Ratra</p><p>H0[i]=68.9; PT[i]=+1.7; NT[i++]=-1.7; // [<xref ref-type="bibr" rid="scirp.112694-ref99">99</xref>] Park &amp; Ratra</p><p>H0[i]=70.1; PT[i]=+1.9; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref99">99</xref>] Park &amp; Ratra</p><p>H0[i]=68.5; PT[i]=+1.8; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref99">99</xref>] Park &amp; Ratra</p><p>H0[i]=69.6; PT[i]=+1.9; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref99">99</xref>] Park &amp; Ratra</p><p>H0[i]=72; PT[i]=+1.9; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref100">100</xref>] Reid</p><p>H0[i]=73.5; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref100">100</xref>] Reid</p><p>H0[i]=74.22; PT[i]=+1.82; NT[i++]=-1.82; // [<xref ref-type="bibr" rid="scirp.112694-ref101">101</xref>] Riess et al.</p><p>H0[i]=74.03; PT[i]=+1.42; NT[i++]=-1.42; // [<xref ref-type="bibr" rid="scirp.112694-ref101">101</xref>] Riess et al.</p><p>H0[i]=72.8; PT[i]=+1.1; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref102">102</xref>] Riess</p><p>H0[i]=74.3; PT[i]=+1; NT[i++]=-1; // [<xref ref-type="bibr" rid="scirp.112694-ref102">102</xref>] Riess</p><p>H0[i]=71.6; PT[i]=+3.8; NT[i++]=-4.9; // [<xref ref-type="bibr" rid="scirp.112694-ref103">103</xref>] Rusu et al.</p><p>H0[i]=67.99; PT[i]=+0.91; NT[i++]=-0.88; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=68.24; PT[i]=+2.39; NT[i++]=-2.33; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=66.79; PT[i]=+2.6; NT[i++]=-2.32; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=66.8; PT[i]=+2.5; NT[i++]=-2.3; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=66.13; PT[i]=+1.38; NT[i++]=-2.09; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=67.1; PT[i]=+2.4; NT[i++]=-2.3; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=68.44; PT[i]=+0.7; NT[i++]=-0.69; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=69.32; PT[i]=+1.42; NT[i++]=-1.42; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=68; PT[i]=+2.27; NT[i++]=-1.94; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=66.6; PT[i]=+2.2; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=67.19; PT[i]=+1; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=66.8; PT[i]=+1.8; NT[i++]=-1.7; // [<xref ref-type="bibr" rid="scirp.112694-ref104">104</xref>] Ryan</p><p>H0[i]=63.13; PT[i]=+6.48; NT[i++]=-6.48; // [<xref ref-type="bibr" rid="scirp.112694-ref105">105</xref>] Saha &amp; Sahoo</p><p>H0[i]=74.2; PT[i]=+2.7; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref106">106</xref>] Shajib et al.</p><p>H0[i]=75; PT[i]=+40; NT[i++]=-32; // [<xref ref-type="bibr" rid="scirp.112694-ref107">107</xref>] Soares-Santos</p><p>H0[i]=78; PT[i]=+96; NT[i++]=-24; // [<xref ref-type="bibr" rid="scirp.112694-ref107">107</xref>] Soares-Santos</p><p>H0[i]=73.1; PT[i]=+0.7; NT[i++]=-0.7; // [<xref ref-type="bibr" rid="scirp.112694-ref108">108</xref>] Taubenberger et al.</p><p>H0[i]=68; PT[i]=+14; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref109">109</xref>] Tiwari et al.</p><p>H0[i]=68; PT[i]=+18; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref109">109</xref>] Tiwari et al.</p><p>H0[i]=73.9; PT[i]=+1; NT[i++]=-1; // [<xref ref-type="bibr" rid="scirp.112694-ref110">110</xref>] Verde et al.</p><p>H0[i]=72.5; PT[i]=+1.2; NT[i++]=-1.2; // [<xref ref-type="bibr" rid="scirp.112694-ref110">110</xref>] Verde et al.</p><p>H0[i]=73.3; PT[i]=+1.7; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref111">111</xref>] Wong et al.</p><p>H0[i]=72.4; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref112">112</xref>] Yuan et al.</p><p>H0[i]=68.36; PT[i]=+0.53; NT[i++]=-0.52; // [<xref ref-type="bibr" rid="scirp.112694-ref113">113</xref>] Zhang &amp; Huang</p><p>H0[i]=64.9; PT[i]=+4.6; NT[i++]=-4.3; // [<xref ref-type="bibr" rid="scirp.112694-ref114">114</xref>] Zeng and Yan</p><p>H0[i]=67.4; PT[i]=+1.1; NT[i++]=-1.2; // [<xref ref-type="bibr" rid="scirp.112694-ref115">115</xref>] Abbott et al.</p><p>H0[i]=69.3; PT[i]=+0.4; NT[i++]=-0.6; // [<xref ref-type="bibr" rid="scirp.112694-ref115">115</xref>] Abbott et al.</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref116">116</xref>] Benetti et al.</p><p>H0[i]=72.5; PT[i]=+2.1; NT[i++]=-2.1; // [<xref ref-type="bibr" rid="scirp.112694-ref117">117</xref>] Bolejko</p><p>H0[i]=68.1; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref117">117</xref>] Bolejko</p><p>H0[i]=76; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref118">118</xref>] Braatz</p><p>H0[i]=69.3; PT[i]=+4.2; NT[i++]=-4.2; // [<xref ref-type="bibr" rid="scirp.112694-ref118">118</xref>] Braatz</p><p>H0[i]=71.9; PT[i]=+7.1; NT[i++]=-7.1; // [<xref ref-type="bibr" rid="scirp.112694-ref119">119</xref>] Cantiello et al.</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref120">120</xref>] Chen</p><p>H0[i]=67.4; PT[i]=+0.5; NT[i++]=-0.5; // [<xref ref-type="bibr" rid="scirp.112694-ref120">120</xref>] Chen</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref121">121</xref>] Choudhury &amp; Choubey</p><p>H0[i]=72.8; PT[i]=+1.6; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref122">122</xref>] Dhawan et al.</p><p>H0[i]=55; PT[i]=+7; NT[i++]=-20;// [<xref ref-type="bibr" rid="scirp.112694-ref123">123</xref>] Di Valentino &amp; Melchiorri</p><p>H0[i]=67.06; PT[i]=+1.68; NT[i++]=-1.68; // [<xref ref-type="bibr" rid="scirp.112694-ref124">124</xref>] Gomez-Valent</p><p>H0[i]=68.9; PT[i]=+1.96; NT[i++]=-1.96; // [<xref ref-type="bibr" rid="scirp.112694-ref124">124</xref>] Gomez-Valent</p><p>H0[i]=68.45; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref124">124</xref>] Gomez-Valent</p><p>H0[i]=73.5; PT[i]=+4.6; NT[i++]=-4.7; // [<xref ref-type="bibr" rid="scirp.112694-ref125">125</xref>] Grillo</p><p>H0[i]=72.8; PT[i]=+4.3; NT[i++]=-4.1; // [<xref ref-type="bibr" rid="scirp.112694-ref125">125</xref>] Grillo</p><p>H0[i]=69.8; PT[i]=+5.3; NT[i++]=-4.1; // [<xref ref-type="bibr" rid="scirp.112694-ref125">125</xref>] Grillo</p><p>H0[i]=70.38; PT[i]=+0.6; NT[i++]=-0.6; // [<xref ref-type="bibr" rid="scirp.112694-ref126">126</xref>] Hoeneisen et al.</p><p>H0[i]=71.17; PT[i]=+1.66; NT[i++]=-1.66; // [<xref ref-type="bibr" rid="scirp.112694-ref127">127</xref>] Lee &amp; Jang</p><p>H0[i]=73.52; PT[i]=+1.62; NT[i++]=-1.62; // [<xref ref-type="bibr" rid="scirp.112694-ref128">128</xref>] Riess et al.</p><p>H0[i]=73.83; PT[i]=+1.48; NT[i++]=-1.48; // [<xref ref-type="bibr" rid="scirp.112694-ref128">128</xref>] Riess et al.</p><p>H0[i]=73.48; PT[i]=+1.66; NT[i++]=-1.66; // [<xref ref-type="bibr" rid="scirp.112694-ref129">129</xref>] Riess et al.</p><p>H0[i]=74.4; PT[i]=+4.9; NT[i++]=-4.9; // [<xref ref-type="bibr" rid="scirp.112694-ref130">130</xref>] Van Putten</p><p>H0[i]=74.5; PT[i]=+7.3; NT[i++]=-7.3; // [<xref ref-type="bibr" rid="scirp.112694-ref130">130</xref>] Van Putten</p><p>H0[i]=74.9; PT[i]=+2.6; NT[i++]=-2.6; // [<xref ref-type="bibr" rid="scirp.112694-ref130">130</xref>] Van Putten</p><p>H0[i]=66.8; PT[i]=+1.9; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref130">130</xref>] Van Putten</p><p>H0[i]=73.75; PT[i]=+1.44; NT[i++]=-1.44; // [<xref ref-type="bibr" rid="scirp.112694-ref130">130</xref>] Van Putten</p><p>H0[i]=70; PT[i]=+12; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref131">131</xref>] Vitale</p><p>H0[i]=67; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref132">132</xref>] Yu et al.</p><p>H0[i]=67.498; PT[i]=+7.97; NT[i++]=-3.278; // [<xref ref-type="bibr" rid="scirp.112694-ref133">133</xref>] Zhang</p><p>H0[i]=70; PT[i]=+12; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref134">134</xref>] Abbott</p><p>H0[i]=72.5; PT[i]=+2.5; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref135">135</xref>] Bethapudi &amp; Desai</p><p>H0[i]=71.9; PT[i]=+2.4; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref136">136</xref>] Bonvin et al.</p><p>H0[i]=69.2; PT[i]=+1.4; NT[i++]=-2.2; // [<xref ref-type="bibr" rid="scirp.112694-ref136">136</xref>] Bonvin et al.</p><p>H0[i]=79; PT[i]=+4.4; NT[i++]=-4.2; // [<xref ref-type="bibr" rid="scirp.112694-ref136">136</xref>] Bonvin et al.</p><p>H0[i]=73.75; PT[i]=+2.11; NT[i++]=-2.11; // [<xref ref-type="bibr" rid="scirp.112694-ref137">137</xref>] Cardona</p><p>H0[i]=67.81; PT[i]=+0.92; NT[i++]=-0.92; // [<xref ref-type="bibr" rid="scirp.112694-ref137">137</xref>] Cardona</p><p>H0[i]=66.93; PT[i]=+0.62; NT[i++]=-0.62; // [<xref ref-type="bibr" rid="scirp.112694-ref137">137</xref>] Cardona</p><p>H0[i]=73.46; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref137">137</xref>] Cardona</p><p>H0[i]=68.3; PT[i]=+2.7; NT[i++]=-2.6; // [<xref ref-type="bibr" rid="scirp.112694-ref138">138</xref>] Chen Yun et al.</p><p>H0[i]=68.4; PT[i]=+2.9; NT[i++]=-3.3; // [<xref ref-type="bibr" rid="scirp.112694-ref138">138</xref>] Chen Yun et al.</p><p>H0[i]=65; PT[i]=+6.6; NT[i++]=-6.6; // [<xref ref-type="bibr" rid="scirp.112694-ref138">138</xref>] Chen Yun et al.</p><p>H0[i]=67.9; PT[i]=+2.4; NT[i++]=-2.4; // [<xref ref-type="bibr" rid="scirp.112694-ref138">138</xref>] Chen Yun et al.</p><p>H0[i]=68; PT[i]=+2.8; NT[i++]=-2.8; // [<xref ref-type="bibr" rid="scirp.112694-ref139">139</xref>] Farooq</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref139">139</xref>] Farooq</p><p>H0[i]=72.72; PT[i]=+1.67; NT[i++]=-1.67; // [<xref ref-type="bibr" rid="scirp.112694-ref140">140</xref>] Feeney et al.</p><p>H0[i]=73.15; PT[i]=+1.78; NT[i++]=-1.78; // [<xref ref-type="bibr" rid="scirp.112694-ref140">140</xref>] Feeney et al.</p><p>H0[i]=67.6; PT[i]=+0.7; NT[i++]=-0.6; // [<xref ref-type="bibr" rid="scirp.112694-ref141">141</xref>] Grieb et al.</p><p>H0[i]=73; PT[i]=+1.75; NT[i++]=-1.75; // [<xref ref-type="bibr" rid="scirp.112694-ref142">142</xref>] Guo &amp; Zhang</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref143">143</xref>] Hjorth et al.</p><p>H0[i]=69.13; PT[i]=+0.24; NT[i++]=-0.24; // [<xref ref-type="bibr" rid="scirp.112694-ref144">144</xref>] Huang and Huang</p><p>H0[i]=71.66; PT[i]=+1.8; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref145">145</xref>] Jang &amp; Lee</p><p>H0[i]=73.72; PT[i]=+2.03; NT[i++]=-2.03; // [<xref ref-type="bibr" rid="scirp.112694-ref145">145</xref>] Jang &amp; Lee</p><p>H0[i]=71.17; PT[i]=+1.66; NT[i++]=-1.66; // [<xref ref-type="bibr" rid="scirp.112694-ref145">145</xref>] Jang &amp; Lee</p><p>H0[i]=66.2; PT[i]=+8.9; NT[i++]=-8.9; // [<xref ref-type="bibr" rid="scirp.112694-ref146">146</xref>] Pritychenko</p><p>H0[i]=67.2; PT[i]=+6.9; NT[i++]=-6.9; // [<xref ref-type="bibr" rid="scirp.112694-ref146">146</xref>] Pritychenko</p><p>H0[i]=69.13; PT[i]=+2.34; NT[i++]=-2.34; // [<xref ref-type="bibr" rid="scirp.112694-ref147">147</xref>] Wang et al.</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref148">148</xref>] Wei &amp; Wu</p><p>H0[i]=69.6; PT[i]=+0.7; NT[i++]=-0.7; // [<xref ref-type="bibr" rid="scirp.112694-ref148">148</xref>] Wei &amp; Wu</p><p>H0[i]=73.1; PT[i]=+5.7; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref149">149</xref>] Wong et al.</p><p>H0[i]=72.5; PT[i]=+3.1; NT[i++]=-3.1; // [<xref ref-type="bibr" rid="scirp.112694-ref150">150</xref>] Zhang et al.</p><p>H0[i]=67.8; PT[i]=+0.9; NT[i++]=-0.9; // [<xref ref-type="bibr" rid="scirp.112694-ref151">151</xref>] Ade et al.</p><p>H0[i]=66; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref152">152</xref>] Gao et al.</p><p>H0[i]=70.1; PT[i]=+0.34; NT[i++]=-0.34; // [<xref ref-type="bibr" rid="scirp.112694-ref153">153</xref>] Ichiki et al.</p><p>H0[i]=66.5; PT[i]=+1.8; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref154">154</xref>] Ludovic et al.</p><p>H0[i]=64.2; PT[i]=+1.9; NT[i++]=-1.9; // [<xref ref-type="bibr" rid="scirp.112694-ref154">154</xref>] Ludovic et al.</p><p>H0[i]=91.8; PT[i]=+5.3; NT[i++]=-5.3; // [<xref ref-type="bibr" rid="scirp.112694-ref155">155</xref>] Moresco et al.</p><p>H0[i]=72.25; PT[i]=+2.51; NT[i++]=-2.51; // [<xref ref-type="bibr" rid="scirp.112694-ref156">156</xref>] Riess et al.</p><p>H0[i]=72.04; PT[i]=+2.67; NT[i++]=-2.67; // [<xref ref-type="bibr" rid="scirp.112694-ref156">156</xref>] Riess et al.</p><p>H0[i]=76.18; PT[i]=+2.37; NT[i++]=-2.37; // [<xref ref-type="bibr" rid="scirp.112694-ref156">156</xref>] Riess et al.</p><p>H0[i]=74.5; PT[i]=+3.27; NT[i++]=-3.27; // [<xref ref-type="bibr" rid="scirp.112694-ref156">156</xref>] Riess et al.</p><p>H0[i]=73.24; PT[i]=+1.74; NT[i++]=-1.74; // [<xref ref-type="bibr" rid="scirp.112694-ref156">156</xref>] Riess et al.</p><p>H0[i]=76.2; PT[i]=+3.4; NT[i++]=-3.4; // [<xref ref-type="bibr" rid="scirp.112694-ref157">157</xref>] Tully et al.</p><p>H0[i]=75; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref157">157</xref>] Tully et al.</p><p>H0[i]=68.17; PT[i]=+1.55; NT[i++]=-1.56; // [<xref ref-type="bibr" rid="scirp.112694-ref158">158</xref>] Cheng &amp; Qing Guo</p><p>H0[i]=68.11; PT[i]=+1.69; NT[i++]=-1.69; // [<xref ref-type="bibr" rid="scirp.112694-ref158">158</xref>] Cheng &amp; Qing Guo</p><p>H0[i]=68.11; PT[i]=+0.86; NT[i++]=-0.86; // [<xref ref-type="bibr" rid="scirp.112694-ref158">158</xref>] Cheng &amp; Qing Guo</p><p>H0[i]=67.7; PT[i]=+1.1; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref159">159</xref>] Cuesta et al.</p><p>H0[i]=69.8; PT[i]=+2.6; NT[i++]=-2.6; // [<xref ref-type="bibr" rid="scirp.112694-ref160">160</xref>] Jang &amp; Lee</p><p>H0[i]=72.2; PT[i]=+3.3; NT[i++]=-3.3; // [<xref ref-type="bibr" rid="scirp.112694-ref160">160</xref>] Jang &amp; Lee</p><p>H0[i]=68.1; PT[i]=+5.9; NT[i++]=-5.9; // [<xref ref-type="bibr" rid="scirp.112694-ref161">161</xref>] Kumar et al.</p><p>H0[i]=73; PT[i]=+26; NT[i++]=-22; // [<xref ref-type="bibr" rid="scirp.112694-ref162">162</xref>] Kuo et al.</p><p>H0[i]=70.6; PT[i]=+2.6; NT[i++]=-2.6; // [<xref ref-type="bibr" rid="scirp.112694-ref163">163</xref>] Rigault et al.</p><p>H0[i]=68.8; PT[i]=+3.3; NT[i++]=-3.3; // [<xref ref-type="bibr" rid="scirp.112694-ref163">163</xref>] Rigault et al.</p><p>H0[i]=67.3; PT[i]=+1.2; NT[i++]=-1.2; // [<xref ref-type="bibr" rid="scirp.112694-ref164">164</xref>] Ade et al.</p><p>H0[i]=70.8; PT[i]=+2.4; NT[i++]=-2.4; // [<xref ref-type="bibr" rid="scirp.112694-ref165">165</xref>] Ben-Dayan et al.</p><p>H0[i]=69.6; PT[i]=+0.7; NT[i++]=-0.7; // [<xref ref-type="bibr" rid="scirp.112694-ref166">166</xref>] Bennett et al.</p><p>H0[i]=64.9; PT[i]=+4.2; NT[i++]=-4.2; // [<xref ref-type="bibr" rid="scirp.112694-ref167">167</xref>] Busti et al.</p><p>H0[i]=72.5; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref168">168</xref>] Efstathiou</p><p>H0[i]=70.6; PT[i]=+3.3; NT[i++]=-3.3; // [<xref ref-type="bibr" rid="scirp.112694-ref168">168</xref>] Efstathiou</p><p>H0[i]=74.1; PT[i]=+2.2; NT[i++]=-2.2; // [<xref ref-type="bibr" rid="scirp.112694-ref169">169</xref>] Lima &amp; Cunha</p><p>H0[i]=70; PT[i]=+2.2; NT[i++]=-2.2; // [<xref ref-type="bibr" rid="scirp.112694-ref170">170</xref>] Bennett et al.</p><p>H0[i]=69.32; PT[i]=+0.8; NT[i++]=-0.8; // [<xref ref-type="bibr" rid="scirp.112694-ref170">170</xref>] Bennett et al.</p><p>H0[i]=68; PT[i]=+4.8; NT[i++]=-4.8; // [<xref ref-type="bibr" rid="scirp.112694-ref171">171</xref>] Braatz et al.</p><p>H0[i]=68; PT[i]=+2.8; NT[i++]=-2.8; // [<xref ref-type="bibr" rid="scirp.112694-ref172">172</xref>] Farooq &amp; Bathra</p><p>H0[i]=73.8; PT[i]=+2.4; NT[i++]=-2.4; // [<xref ref-type="bibr" rid="scirp.112694-ref172">172</xref>] Farooq &amp; Bathra</p><p>H0[i]=69.7; PT[i]=+2.4; NT[i++]=-2.4; // [<xref ref-type="bibr" rid="scirp.112694-ref173">173</xref>] Hinshaw et al.</p><p>H0[i]=70.4; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref173">173</xref>] Hinshaw et al.</p><p>H0[i]=69.33; PT[i]=+0.88; NT[i++]=-0.88; // [<xref ref-type="bibr" rid="scirp.112694-ref173">173</xref>] Hinshaw et al.</p><p>H0[i]=70.2; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref173">173</xref>] Hinshaw et al.</p><p>H0[i]=70; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref174">174</xref>] Humphreys et al.</p><p>H0[i]=68; PT[i]=+9; NT[i++]=-9; // [<xref ref-type="bibr" rid="scirp.112694-ref175">175</xref>] Kuo et al.</p><p>H0[i]=49.97; PT[i]=+0.19; NT[i++]=-0.19; // [<xref ref-type="bibr" rid="scirp.112694-ref176">176</xref>] Pietrzynski et al.</p><p>H0[i]=68.9; PT[i]=+7.1; NT[i++]=-7.1; // [<xref ref-type="bibr" rid="scirp.112694-ref177">177</xref>] Reid et al.</p><p>H0[i]=72.1; PT[i]=+3.2; NT[i++]=-2.3; // [<xref ref-type="bibr" rid="scirp.112694-ref178">178</xref>] Salvatelli et al.</p><p>H0[i]=74.1; PT[i]=+2.1; NT[i++]=-2.1; // [<xref ref-type="bibr" rid="scirp.112694-ref179">179</xref>] Scowcroft et al.</p><p>H0[i]=69; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref180">180</xref>] Sereno and Pacificz</p><p>H0[i]=80; PT[i]=+5.8; NT[i++]=-5.7; // [<xref ref-type="bibr" rid="scirp.112694-ref181">181</xref>] Suyu et al.</p><p>H0[i]=75.2; PT[i]=+4.4; NT[i++]=-4.2; // [<xref ref-type="bibr" rid="scirp.112694-ref181">181</xref>] Suyu et al.</p><p>H0[i]=73.1; PT[i]=+2.4; NT[i++]=-3.6; // [<xref ref-type="bibr" rid="scirp.112694-ref181">181</xref>] Suyu et al.</p><p>H0[i]=74.4; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref182">182</xref>] Tully et al.</p><p>H0[i]=71.3; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref183">183</xref>] Xia et al.</p><p>H0[i]=73.8; PT[i]=+2.4; NT[i++]=-2.4; // [<xref ref-type="bibr" rid="scirp.112694-ref184">184</xref>] Calabrese et al.</p><p>H0[i]=68; PT[i]=+2.8; NT[i++]=-2.8; // [<xref ref-type="bibr" rid="scirp.112694-ref184">184</xref>] Calabrese et al.</p><p>H0[i]=69.7; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref184">184</xref>] Calabrese et al.</p><p>H0[i]=74.3; PT[i]=+3.1; NT[i++]=-3.1; // [<xref ref-type="bibr" rid="scirp.112694-ref185">185</xref>] Chavez</p><p>H0[i]=67; PT[i]=+3.2; NT[i++]=-3.2; // [<xref ref-type="bibr" rid="scirp.112694-ref186">186</xref>] Colless et al.</p><p>H0[i]=74.3; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref187">187</xref>] Freedman et al.</p><p>H0[i]=70.2; PT[i]=+0.14; NT[i++]=-0.14; // [<xref ref-type="bibr" rid="scirp.112694-ref188">188</xref>] Pozzo</p><p>H0[i]=75.4; PT[i]=+2.9; NT[i++]=-2.9; // [<xref ref-type="bibr" rid="scirp.112694-ref189">189</xref>] Riess et al.</p><p>H0[i]=56; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref190">190</xref>] Wang</p><p>H0[i]=68; PT[i]=+5.5; NT[i++]=-5.5; // [<xref ref-type="bibr" rid="scirp.112694-ref191">191</xref>] Chen &amp; Ratra</p><p>H0[i]=67; PT[i]=+3.2; NT[i++]=-3.2; // [<xref ref-type="bibr" rid="scirp.112694-ref192">192</xref>] Beutler et al.</p><p>H0[i]=71; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref193">193</xref>] Jarosik et al.</p><p>H0[i]=70.4; PT[i]=+1.3; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref193">193</xref>] Jarosik et al.</p><p>H0[i]=74.8; PT[i]=+3.1; NT[i++]=-3.1; // [<xref ref-type="bibr" rid="scirp.112694-ref194">194</xref>] Riess et al.</p><p>H0[i]=74.4; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref194">194</xref>] Riess et al.</p><p>H0[i]=73.8; PT[i]=+2.4; NT[i++]=-2.4; // [<xref ref-type="bibr" rid="scirp.112694-ref194">194</xref>] Riess et al.</p><p>H0[i]=73; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref195">195</xref>] Freedman &amp; Madore</p><p>H0[i]=66; PT[i]=+6; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref196">196</xref>] Paraficz et Hjorth</p><p>H0[i]=76; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref196">196</xref>] Paraficz et Hjorth</p><p>H0[i]=70.6; PT[i]=+3.1; NT[i++]=-3.1; // [<xref ref-type="bibr" rid="scirp.112694-ref197">197</xref>] Suyu et al.</p><p>H0[i]=69.7; PT[i]=+4.9; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref197">197</xref>] Suyu et al.</p><p>H0[i]=70.5; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref198">198</xref>] Hinshaw et al.</p><p>H0[i]=71.9; PT[i]=+2.6; NT[i++]=-2.7; // [<xref ref-type="bibr" rid="scirp.112694-ref198">198</xref>] Hinshaw et al.</p><p>H0[i]=70.5; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref199">199</xref>] Komatsu et al.</p><p>H0[i]=70.4; PT[i]=+1.4; NT[i++]=-1.4; // [<xref ref-type="bibr" rid="scirp.112694-ref199">199</xref>] Komatsu et al.</p><p>H0[i]=70.9; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref199">199</xref>] Komatsu et al.</p><p>H0[i]=70.1; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref199">199</xref>] Komatsu et al.</p><p>H0[i]=74.2; PT[i]=+3.6; NT[i++]=-3.6; // [<xref ref-type="bibr" rid="scirp.112694-ref200">200</xref>] Riess et al.</p><p>H0[i]=84.2; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref201">201</xref>] Russell</p><p>H0[i]=83.4; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref201">201</xref>] Russell</p><p>H0[i]=88; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref201">201</xref>] Russell</p><p>H0[i]=61.7; PT[i]=+1.2; NT[i++]=-1.1; // [<xref ref-type="bibr" rid="scirp.112694-ref202">202</xref>] Leith et al.</p><p>H0[i]=67; PT[i]=+13; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref203">203</xref>] Vuissoz et al.</p><p>H0[i]=63; PT[i]=+7; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref203">203</xref>] Vuissoz et al.</p><p>H0[i]=70; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref204">204</xref>] Oguri</p><p>H0[i]=68; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref204">204</xref>] Oguri</p><p>H0[i]=73.5; PT[i]=+3.2; NT[i++]=-3.2; // [<xref ref-type="bibr" rid="scirp.112694-ref205">205</xref>] Spergel et al.</p><p>H0[i]=73.2; PT[i]=+3.1; NT[i++]=-3.2; // [<xref ref-type="bibr" rid="scirp.112694-ref205">205</xref>] Spergel et al.</p><p>H0[i]=70.4; PT[i]=+1.5; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref205">205</xref>] Spergel et al.</p><p>H0[i]=76.9; PT[i]=+3.9; NT[i++]=-3.4; // [<xref ref-type="bibr" rid="scirp.112694-ref206">206</xref>] Bonamente et al.</p><p>H0[i]=73.7; PT[i]=+4.6; NT[i++]=-3.8; // [<xref ref-type="bibr" rid="scirp.112694-ref206">206</xref>] Bonamente et al.</p><p>H0[i]=77.6; PT[i]=+4.8; NT[i++]=-4.3; // [<xref ref-type="bibr" rid="scirp.112694-ref206">206</xref>] Bonamente et al.</p><p>H0[i]=70.8; PT[i]=+1.9; NT[i++]=-1.8; // [<xref ref-type="bibr" rid="scirp.112694-ref207">207</xref>] H&#252;tsi</p><p>H0[i]=74.92; PT[i]=+2.28; NT[i++]=-2.28; // [<xref ref-type="bibr" rid="scirp.112694-ref208">208</xref>] Ngeow and Kanbur</p><p>H0[i]=74.37; PT[i]=+2.27; NT[i++]=-2.27; // [<xref ref-type="bibr" rid="scirp.112694-ref208">208</xref>] Ngeow and Kanbur</p><p>H0[i]=62.3; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref209">209</xref>] Sandage et al.</p><p>H0[i]=60.9; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref209">209</xref>] Sandage et al.</p><p>H0[i]=60.7; PT[i]=+1.5; NT[i++]=-1.5; // [<xref ref-type="bibr" rid="scirp.112694-ref209">209</xref>] Sandage et al.</p><p>H0[i]=72; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref210">210</xref>] Wang et al.</p><p>H0[i]=73.2; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref211">211</xref>] Gibson &amp; Brook</p><p>H0[i]=75; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref212">212</xref>] Hamuy</p><p>H0[i]=65; PT[i]=+12; NT[i++]=-12; // [<xref ref-type="bibr" rid="scirp.112694-ref212">212</xref>] Hamuy</p><p>H0[i]=58; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref213">213</xref>] Magain</p><p>H0[i]=58; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref214">214</xref>] Olivares et al.</p><p>H0[i]=73; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref215">215</xref>] Riess</p><p>H0[i]=69; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref216">216</xref>] Schmidt et al.</p><p>H0[i]=66; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref217">217</xref>] Stritzinger et al.</p><p>H0[i]=78; PT[i]=+9; NT[i++]=-9; // [<xref ref-type="bibr" rid="scirp.112694-ref217">217</xref>] Stritzinger et al.</p><p>H0[i]=67; PT[i]=+30; NT[i++]=-18; // [<xref ref-type="bibr" rid="scirp.112694-ref218">218</xref>] Udomprasert et al.</p><p>H0[i]=64; PT[i]=+7; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref219">219</xref>] Boffi &amp; Riess</p><p>H0[i]=33; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref220">220</xref>] Dumin</p><p>H0[i]=69; PT[i]=+12; NT[i++]=-12; // [<xref ref-type="bibr" rid="scirp.112694-ref221">221</xref>] Jimenez et al.</p><p>H0[i]=75; PT[i]=+7; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref222">222</xref>] Koopmans</p><p>H0[i]=70; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref223">223</xref>] Mei et al.</p><p>H0[i]=68; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref223">223</xref>] Mei et al.</p><p>H0[i]=68; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref223">223</xref>] Mei et al.</p><p>H0[i]=71; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref223">223</xref>] Mei et al.</p><p>H0[i]=77; PT[i]=+19; NT[i++]=-15; // [<xref ref-type="bibr" rid="scirp.112694-ref224">224</xref>] Saunders et al.</p><p>H0[i]=85; PT[i]=+20; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref224">224</xref>] Saunders et al.</p><p>H0[i]=72; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref225">225</xref>] Spergel et al.</p><p>H0[i]=71; PT[i]=+4; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref225">225</xref>] Spergel et al.</p><p>H0[i]=63; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref226">226</xref>] Fassnacht et al.</p><p>H0[i]=72; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref227">227</xref>] Freedman</p><p>H0[i]=57; PT[i]=+23; NT[i++]=-16; // [<xref ref-type="bibr" rid="scirp.112694-ref228">228</xref>] Grainge et al.</p><p>H0[i]=48; PT[i]=+7; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref229">229</xref>] Kochanek</p><p>H0[i]=71; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref229">229</xref>] Kochanek</p><p>H0[i]=72; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref229">229</xref>] Kochanek</p><p>H0[i]=62; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref229">229</xref>] Kochanek</p><p>H0[i]=75; PT[i]=+8; NT[i++]=-8;// [<xref ref-type="bibr" rid="scirp.112694-ref230">230</xref>] Tikhonov &amp; Galazoutdinova</p><p>H0[i]=81; PT[i]=+5; NT[i++]=-5;// [<xref ref-type="bibr" rid="scirp.112694-ref230">230</xref>] Tikhonov &amp; Galazoutdinova</p><p>H0[i]=59; PT[i]=+15; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref231">231</xref>] Treu &amp; Koopmans</p><p>H0[i]=71; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref232">232</xref>] Freedman et al.</p><p>H0[i]=71; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref232">232</xref>] Freedman et al.</p><p>H0[i]=70; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref232">232</xref>] Freedman et al.</p><p>H0[i]=72; PT[i]=+9; NT[i++]=-9; // [<xref ref-type="bibr" rid="scirp.112694-ref232">232</xref>] Freedman et al.</p><p>H0[i]=82; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref232">232</xref>] Freedman et al.</p><p>H0[i]=72; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref232">232</xref>] Freedman et al.</p><p>H0[i]=65; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref233">233</xref>] Itoh</p><p>H0[i]=76; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref234">234</xref>] Jensen et al.</p><p>H0[i]=72; PT[i]=+2.3; NT[i++]=-2.3; // [<xref ref-type="bibr" rid="scirp.112694-ref234">234</xref>] Jensen et al.</p><p>H0[i]=65; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref235">235</xref>] Koopmans et al.</p><p>H0[i]=71; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref236">236</xref>] Liu &amp; Graham</p><p>H0[i]=64; PT[i]=+14; NT[i++]=-18; // [<xref ref-type="bibr" rid="scirp.112694-ref237">237</xref>] Mason et al.</p><p>H0[i]=66; PT[i]=+14; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref237">237</xref>] Mason et al.</p><p>H0[i]=70; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref238">238</xref>] Mei et al.</p><p>H0[i]=69; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref239">239</xref>] Tonry</p><p>H0[i]=71; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref240">240</xref>] Willick &amp; Puneet</p><p>H0[i]=63; PT[i]=+4.3; NT[i++]=-4.3; // [<xref ref-type="bibr" rid="scirp.112694-ref241">241</xref>] Xiao-Feng et al.</p><p>H0[i]=69; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref242">242</xref>] Ferrarese et al.</p><p>H0[i]=68; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref243">243</xref>] Gibson et al.</p><p>H0[i]=71; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref244">244</xref>] Mould et al.</p><p>H0[i]=68; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref244">244</xref>] Mould et al.</p><p>H0[i]=71; PT[i]=+4; NT[i++]=-4; // [<xref ref-type="bibr" rid="scirp.112694-ref245">245</xref>] Sakai et al.</p><p>H0[i]=77; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref246">246</xref>] Tikhonov et al.</p><p>H0[i]=69; PT[i]=+12; NT[i++]=-19; // [<xref ref-type="bibr" rid="scirp.112694-ref247">247</xref>] Biggs et al.</p><p>H0[i]=69; PT[i]=+18; NT[i++]=-12; // [<xref ref-type="bibr" rid="scirp.112694-ref248">248</xref>] Chae KH</p><p>H0[i]=74; PT[i]=+18; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref248">248</xref>] Chae KH</p><p>H0[i]=42; PT[i]=+9; NT[i++]=-9; // [<xref ref-type="bibr" rid="scirp.112694-ref249">249</xref>] Collier et al.</p><p>H0[i]=73; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref250">250</xref>] Freedman et al.</p><p>H0[i]=64; PT[i]=+8; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref251">251</xref>] Jha et al.</p><p>H0[i]=85; PT[i]=+27; NT[i++]=-23; // [<xref ref-type="bibr" rid="scirp.112694-ref252">252</xref>] Mason &amp; Myers</p><p>H0[i]=61; PT[i]=+15; NT[i++]=-14; // [<xref ref-type="bibr" rid="scirp.112694-ref252">252</xref>] Mason &amp; Myers</p><p>H0[i]=61; PT[i]=+23; NT[i++]=-21; // [<xref ref-type="bibr" rid="scirp.112694-ref252">252</xref>] Mason &amp; Myers</p><p>H0[i]=80; PT[i]=+19; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref252">252</xref>] Mason &amp; Myers</p><p>H0[i]=68; PT[i]=+21; NT[i++]=-19; // [<xref ref-type="bibr" rid="scirp.112694-ref252">252</xref>] Mason &amp; Myers</p><p>H0[i]=71; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref252">252</xref>] Mason &amp; Myers</p><p>H0[i]=86; PT[i]=+24; NT[i++]=-24; // [<xref ref-type="bibr" rid="scirp.112694-ref253">253</xref>] Mazumdar &amp; Narasimba</p><p>H0[i]=67; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref254">254</xref>] Tanvir et al.</p><p>H0[i]=62.9; PT[i]=+1.6; NT[i++]=-1.6; // [<xref ref-type="bibr" rid="scirp.112694-ref255">255</xref>] Tripp &amp; Branch</p><p>H0[i]=62; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref255">255</xref>] Tripp &amp; Branch</p><p>H0[i]=60; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref256">256</xref>] Branch</p><p>H0[i]=66; PT[i]=+15; NT[i++]=-14; // [<xref ref-type="bibr" rid="scirp.112694-ref257">257</xref>] Goicoechea et al.</p><p>H0[i]=77; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref258">258</xref>] Harris et al.</p><p>H0[i]=47; PT[i]=+23; NT[i++]=-15; // [<xref ref-type="bibr" rid="scirp.112694-ref259">259</xref>] Hughes &amp; Birkinshaw</p><p>H0[i]=82; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref260">260</xref>] Lauer et al.</p><p>H0[i]=89; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref260">260</xref>] Lauer et al.</p><p>H0[i]=65.2; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref261">261</xref>] Riess et al.</p><p>H0[i]=63.8; PT[i]=+1.3; NT[i++]=-1.3; // [<xref ref-type="bibr" rid="scirp.112694-ref261">261</xref>] Riess et al.</p><p>H0[i]=55; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref262">262</xref>] Tammann &amp; Labhardt</p><p>H0[i]=60; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref263">263</xref>] Tripp</p><p>H0[i]=70; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref264">264</xref>] Giovanelli</p><p>H0[i]=76; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref264">264</xref>] Giovanelli</p><p>H0[i]=67; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref264">264</xref>] Giovanelli</p><p>H0[i]=75; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref265">265</xref>] Gregg</p><p>H0[i]=67; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref266">266</xref>] Hjorth &amp; Tanvir</p><p>H0[i]=70; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref266">266</xref>] Hjorth &amp; Tanvir</p><p>H0[i]=60; PT[i]=+40; NT[i++]=-23; // [<xref ref-type="bibr" rid="scirp.112694-ref267">267</xref>] Holzapfel et al.</p><p>H0[i]=78; PT[i]=+34; NT[i++]=-28; // [<xref ref-type="bibr" rid="scirp.112694-ref267">267</xref>] Holzapfel et al.</p><p>H0[i]=78; PT[i]=+60; NT[i++]=-40; // [<xref ref-type="bibr" rid="scirp.112694-ref267">267</xref>] Holzapfel et al.</p><p>H0[i]=58; PT[i]=+10; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref268">268</xref>] Hoyle et al.</p><p>H0[i]=74; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref269">269</xref>] Schechter</p><p>H0[i]=52.5; PT[i]=+2.5; NT[i++]=-2.5; // [<xref ref-type="bibr" rid="scirp.112694-ref270">270</xref>] Sciama</p><p>H0[i]=54.8; PT[i]=+0.3; NT[i++]=-0.3; // [<xref ref-type="bibr" rid="scirp.112694-ref270">270</xref>] Sciama</p><p>H0[i]=81; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref271">271</xref>] Tonry et al.</p><p>H0[i]=69; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref272">272</xref>] Amendola</p><p>H0[i]=80; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref272">272</xref>] Amendola</p><p>H0[i]=49.5; PT[i]=+4.5; NT[i++]=-4.5; // [<xref ref-type="bibr" rid="scirp.112694-ref273">273</xref>] Biesiada</p><p>H0[i]=65; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref274">274</xref>] Forbes et al.</p><p>H0[i]=103; PT[i]=+59; NT[i++]=-28; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=82; PT[i]=+56; NT[i++]=-24; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=60; PT[i]=+24; NT[i++]=-13; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=51; PT[i]=+10; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=33; PT[i]=+22; NT[i++]=-9; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=74; PT[i]=+26; NT[i++]=-15; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=63; PT[i]=+28; NT[i++]=-15; // [<xref ref-type="bibr" rid="scirp.112694-ref275">275</xref>] Kobayashi</p><p>H0[i]=80; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref276">276</xref>] Mallik</p><p>H0[i]=87; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref276">276</xref>] Mallik</p><p>H0[i]=55; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref277">277</xref>] Schaefer</p><p>H0[i]=56; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref277">277</xref>] Schaefer</p><p>H0[i]=82.5; PT[i]=+5.9; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref278">278</xref>] Grogin &amp; Narayan</p><p>H0[i]=82.5; PT[i]=+8.7; NT[i++]=-5.6; // [<xref ref-type="bibr" rid="scirp.112694-ref278">278</xref>] Grogin &amp; Narayan</p><p>H0[i]=71; PT[i]=+30; NT[i++]=-25; // [<xref ref-type="bibr" rid="scirp.112694-ref279">279</xref>] Herbig</p><p>H0[i]=74.6; PT[i]=+47; NT[i++]=-33; // [<xref ref-type="bibr" rid="scirp.112694-ref280">280</xref>] Holzapfel et al.</p><p>H0[i]=38; PT[i]=+18; NT[i++]=-16; // [<xref ref-type="bibr" rid="scirp.112694-ref281">281</xref>] Jones</p><p>H0[i]=80; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref282">282</xref>] Kennicutt Jr et al.</p><p>H0[i]=73; PT[i]=+11; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=81; PT[i]=+11; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=84; PT[i]=+16; NT[i++]=-16; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=76; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=82; PT[i]=+11; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=71; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=80; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref283">283</xref>] Mould</p><p>H0[i]=80; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref284">284</xref>] Nakamura &amp; Suto</p><p>H0[i]=58; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref285">285</xref>] Rephaeli</p><p>H0[i]=51; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref286">286</xref>] Schaefer</p><p>H0[i]=61; PT[i]=+12; NT[i++]=-12; // [<xref ref-type="bibr" rid="scirp.112694-ref286">286</xref>] Schaefer</p><p>H0[i]=26; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref286">286</xref>] Schaefer</p><p>H0[i]=69; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref287">287</xref>] Tanvir et al.</p><p>H0[i]=78; PT[i]=+11; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref288">288</xref>] Whitmore &amp; Schweizer</p><p>H0[i]=65; PT[i]=+25; NT[i++]=-25; // [<xref ref-type="bibr" rid="scirp.112694-ref289">289</xref>] Birkinshaw &amp; Hughes</p><p>H0[i]=55; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref289">289</xref>] Birkinshaw &amp; Hughes</p><p>H0[i]=80; PT[i]=+17; NT[i++]=-17; // [<xref ref-type="bibr" rid="scirp.112694-ref290">290</xref>] Freedman</p><p>H0[i]=84; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref291">291</xref>] Lu et al.</p><p>H0[i]=73; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref292">292</xref>] Schmidt &amp; Kirshner</p><p>H0[i]=90; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref293">293</xref>] Tully</p><p>H0[i]=43.5; PT[i]=+2.7; NT[i++]=-2.7; // [<xref ref-type="bibr" rid="scirp.112694-ref294">294</xref>] Duemmler</p><p>H0[i]=77; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref295">295</xref>] Lauer &amp; Postman</p><p>H0[i]=51; PT[i]=+5; NT[i++]=-5; // [<xref ref-type="bibr" rid="scirp.112694-ref295">295</xref>] Lauer &amp; Postman</p><p>H0[i]=75; PT[i]=+30; NT[i++]=-30; // [<xref ref-type="bibr" rid="scirp.112694-ref296">296</xref>] Leibundgut &amp; Pinto</p><p>H0[i]=40; PT[i]=+9; NT[i++]=-9; // [<xref ref-type="bibr" rid="scirp.112694-ref297">297</xref>] Birkinshaw</p><p>H0[i]=45; PT[i]=+12; NT[i++]=-12; // [<xref ref-type="bibr" rid="scirp.112694-ref297">297</xref>] Birkinshaw</p><p>H0[i]=82; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref298">298</xref>] Tonry</p><p>H0[i]=52; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref299">299</xref>] Sandage &amp; Tammann</p><p>H0[i]=45; PT[i]=+3; NT[i++]=-3; // [<xref ref-type="bibr" rid="scirp.112694-ref299">299</xref>] Sandage &amp; Tammann</p><p>H0[i]=73; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref300">300</xref>] Visvanathan</p><p>H0[i]=50; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref301">301</xref>] Sandage &amp; Tammann</p><p>H0[i]=52; PT[i]=+2; NT[i++]=-2; // [<xref ref-type="bibr" rid="scirp.112694-ref301">301</xref>] Sandage &amp; Tammann</p><p>H0[i]=50; PT[i]=+7; NT[i++]=-7; // [<xref ref-type="bibr" rid="scirp.112694-ref301">301</xref>] Sandage &amp; Tammann</p><p>H0[i]=67; PT[i]=+10; NT[i++]=-10; // [<xref ref-type="bibr" rid="scirp.112694-ref302">302</xref>] Dressler</p><p>H0[i]=74.3; PT[i]=+11; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref304">304</xref>] Visvanathan</p><p>H0[i]=74.3; PT[i]=+11; NT[i++]=-11; // [<xref ref-type="bibr" rid="scirp.112694-ref305">305</xref>] Hanes</p><p>H0[i]=76; PT[i]=+8; NT[i++]=-8; // [<xref ref-type="bibr" rid="scirp.112694-ref306">306</xref>] Bottinelli &amp; Gouguenheim</p><p>H0[i]=50.3; PT[i]=+4.3; NT[i++]=-4.3; // [<xref ref-type="bibr" rid="scirp.112694-ref307">307</xref>] Sandage &amp; Tammann</p><p>H0[i]=56.9; PT[i]=+3.4; NT[i++]=-3.4; // [<xref ref-type="bibr" rid="scirp.112694-ref308">308</xref>] Sandage &amp; Tammann</p><p>H0[i]=57; PT[i]=+6; NT[i++]=-6; // [<xref ref-type="bibr" rid="scirp.112694-ref309">309</xref>] Sandage &amp; Tammann</p><p>H0[i]=55.5; PT[i]=+8.7; NT[i]=-8.7; // [<xref ref-type="bibr" rid="scirp.112694-ref310">310</xref>] Sandage &amp; Tammann</p><p>//Creates an H0 array that contains all the extremities of the tolerance ranges</p><p>for (i=0;i&lt;=nbH0-1;i++) {</p><p>H0[i+nbH0]=H0[i]+PT[i]; Variation[i+nbH0]=PT[i];</p><p>H0[i]=H0[i]+NT[i]; Variation[i]=NT[i]; }</p><p>//Sorts H0 array in ascending order with corresponding Variation of tolerance</p><p>for (j=0;j&lt;=2*nbH0-2;j++) {</p><p>for (i=j+1;i&lt;=2*nbH0-1;i++) {</p><p>if (H0[i]</p><p>DH0=H0[j]; DSgn=Variation[j]; H0[j]=H0[i];</p><p>Variation[j]=Variation[i]; H0[i]=DH0; Variation[i]=DSgn; } } }</p><p>for (i=0;i&lt;=2*nbH0-1;i++) { //Builds the nbCrossings array</p><p>if (i==0) { nbCrossings[i]=1; }</p><p>else {</p><p>if (Variation[i]&lt;0) {nbCrossings[i]=nbCrossings[i-1]+1;}</p><p>if (Variation[i]&gt;0) {nbCrossings[i]=nbCrossings[i-1]-1;}</p><p>if (H0[i]==H0[i-1]) {</p><p>j=i; DeltaCrossings=0;</p><p>do {</p><p>if (Variation[j]&lt;0) {DeltaCrossings=DeltaCrossings+1;}</p><p>if (Variation[j]&gt;0) {DeltaCrossings=DeltaCrossings-1;}</p><p>j=j-1; } while (H0[j]==H0[i]);</p><p>for(k=i;k&gt;j;k--) {nbCrossings[k]=nbCrossings[j]+DeltaCrossings;}</p><p>} } } } //End of CreateTableOfCrossingH0Ranges</p><p>//***Function that returns the y coordinate corresponding to x for non</p><p>//***centered Gaussian curve</p><p>double GaussianCurve(double x, double Mean, double Sigma, double Multiplier) {</p><p>double y; //Coordinate y corresponding to x for a non centered Gaussian</p><p>y=(Multiplier/(Sigma*Sqrt(2*Pi)))*exp(-0.5*Sqr((x-Mean)/Sigma));</p><p>return y; } //End of CreateApproximativeCurve</p><p>//***These are the best Gaussians to fit the nbCrossing array as a function of H0***</p><p>double FindsGaussianCurvesLS(double Mean[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>],double Sigma[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>], double Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>]) {</p><p>int i,j; /*Counters*/ double LS = 0; //Least square</p><p>double Sum; //Sum of the 5 Gaussien curve for a specific H0 value</p><p>for (j=0;j&lt;=2*nbH0-1;j++) {</p><p>Sum=0;</p><p>for (i=0;i&lt;=4;i++) {</p><p>Sum=Sum+GaussianCurve(H0[j],Mean[i],Sigma[i],Multiplier[i]); }</p><p>//We give a heavier weight to any error between 69.2 and 72.1 to</p><p>// model the gap between these values</p><p>if ((H0[i]&gt;=69.2)&amp;&amp;(H0[i]&lt;=72.1)) {</p><p>LS=LS+10*(Sqr(nbCrossings[j]-Sum));}</p><p>else { LS=LS+Sqr(nbCrossings[j]-Sum); }</p><p>} return LS; } //End of FindsGaussianCurvesLS</p><p>//***This function finds the best Gaussians to fit the real curve</p><p>void FindsBestGaussiansToFitRealCurve(void) {</p><p>int i; //Counter</p><p>double DMean[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>],DSigma[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>],DMultiplier[<xref ref-type="bibr" rid="scirp.112694-ref5">5</xref>]; //Dummy arrays</p><p>double LS, PLS; //Least Square and Previous Least Square</p><p>double StepMean = 0.1, StepSigma = 0.1, StepMultiplier = 0.1; //Variations</p><p>int nbMeanNotImproved = 0; //Tells how many times not improved</p><p>int nbSigmaNotImproved = 0; //Tells how many times not improved</p><p>int nbMultiplierNotImproved = 0; //Tells how many times not improved</p><p>//Starting values (approximative values only)</p><p>Mean[<xref ref-type="bibr" rid="scirp.112694-ref0">0</xref>]=71; Sigma[<xref ref-type="bibr" rid="scirp.112694-ref0">0</xref>]=1; Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref0">0</xref>]=-280;</p><p>Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]=68; Sigma[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]=17; Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]=3800;</p><p>Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]; Sigma[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=3; Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=880;</p><p>Mean[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]=73; Sigma[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]=7; Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]=1200;</p><p>Mean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=Mean[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]; Sigma[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=2; Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=470;</p><p>//Fills the 3 dummy arrays DMean, DSigma and DMultiplier</p><p>//with the same values than the arrays Mean, Sigma and Multiplier</p><p>for(i=0;i&lt;=4;i++) {</p><p>DMean[i]=Mean[i]; DSigma[i]=Sigma[i]; DMultiplier[i]=Multiplier[i]; }</p><p>//Tries to find the 5 best Gaussians to fit the curve</p><p>do {</p><p>for (i=0;i&lt;=4;i++) {</p><p>//We improve Mean[i], but we force</p><p>//Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>] = Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>] &amp; Mean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>] = Mean[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]</p><p>if ((i!=2)&amp;&amp;(i!=4)) {</p><p>PLS=FindsGaussianCurvesLS(Mean,Sigma,Multiplier);</p><p>DMean[i]=Mean[i]+StepMean;</p><p>if (i==1) {DMean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=DMean[i];}</p><p>if (i==3) {DMean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=DMean[i];}</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>if (LS</p><p>Mean[i]=DMean[i];</p><p>if (i==1) {Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=DMean[i];}</p><p>if (i==3) {Mean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=DMean[i];}</p><p>nbMeanNotImproved=0; }</p><p>else {</p><p>DMean[i]=Mean[i]-StepMean;</p><p>if (i==1) {DMean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=DMean[i];}</p><p>if (i==3) {DMean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=DMean[i];}</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>if (LS</p><p>Mean[i]=DMean[i];</p><p>if (i==1) {Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=DMean[i];}</p><p>if (i==3) {Mean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=DMean[i];}</p><p>nbMeanNotImproved=0; }</p><p>else {</p><p>DMean[i]=Mean[i];</p><p>if (i==1) {DMean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=DMean[i];}</p><p>if (i==3) {DMean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]=DMean[i];}</p><p>nbMeanNotImproved++;</p><p>if (nbMeanNotImproved&gt;=100) {</p><p>nbMeanNotImproved=0; StepMean=StepMean/10; } } } }</p><p>//We try to improve Sigma[i]</p><p>PLS=FindsGaussianCurvesLS(Mean,Sigma,Multiplier);</p><p>DSigma[i]=Sigma[i]+StepSigma;</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>if (LS</p><p>else {</p><p>DSigma[i]=Sigma[i]-StepSigma;</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>if (LS</p><p>Sigma[i]=DSigma[i]; nbSigmaNotImproved=0; }</p><p>else {</p><p>DSigma[i]=Sigma[i]; nbSigmaNotImproved++;</p><p>if (nbSigmaNotImproved&gt;=100) {</p><p>nbSigmaNotImproved=0; StepSigma=StepSigma/10; } } }</p><p>//We try to improve Multiplier[i]</p><p>PLS=FindsGaussianCurvesLS(Mean,Sigma,Multiplier);</p><p>DMultiplier[i]=Multiplier[i]+StepMultiplier;</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>if (LS</p><p>Multiplier[i]=DMultiplier[i]; nbMultiplierNotImproved=0; }</p><p>else {</p><p>DMultiplier[i]=Multiplier[i]-StepMultiplier;</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>if (LS</p><p>Multiplier[i]=DMultiplier[i]; nbMultiplierNotImproved=0; }</p><p>else {</p><p>DMultiplier[i]=Multiplier[i]; nbMultiplierNotImproved++;</p><p>if (nbMultiplierNotImproved&gt;=100) {</p><p>nbMultiplierNotImproved=0;</p><p>StepMultiplier=StepMultiplier/10; } } } }</p><p>LS=FindsGaussianCurvesLS(DMean,DSigma,DMultiplier);</p><p>} while (LS&gt;=22000); //Sets a stop point</p><p>for(i=0;i&lt;=4;i++) {</p><p>printf(&quot;\n Mean[%i]=%10lf Sigma[%i]=%10lf Multiplier[%i]=%10lf&quot;,</p><p>i,Mean[i],i,Sigma[i],i,Multiplier[i]);</p><p>} } //End of FindsBestGaussiansToFitRealCurve</p><p>//***The function begins by shifting Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>] and Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>] of the two</p><p>//***Gaussian curves that are around H0=69.2km/(s*MParsec) to</p><p>//***H0=72.1km/(s*MParsec) with a theoretical factor of 1.042516951. Then</p><p>//***the function that modifies the global H0 array builds the summation of</p><p>//***the 4 positive Gaussian curves.</p><p>void CreatesFinalGaussianCurve(void) {</p><p>int i; //Dummy index value</p><p>//We shift Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>] and Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>] with a theoretical factor of 1.042516951</p><p>Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]=Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]*1.042516951; Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]=Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>];</p><p>//We omit i=0 to remove the negative Gaussian curve</p><p>for(i=1;i&lt;=nbH0*2-1;i++) {</p><p>nbCrossings[i]=GaussianCurve(H0[i],Mean[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>],Sigma[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>],Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref1">1</xref>]);</p><p>nbCrossings[i]=nbCrossings[i]+GaussianCurve(H0[i],Mean[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>],Sigma[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>],</p><p>Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref2">2</xref>]);</p><p>nbCrossings[i]=nbCrossings[i]+GaussianCurve(H0[i],Mean[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>],Sigma[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>],</p><p>Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref3">3</xref>]);</p><p>nbCrossings[i]=nbCrossings[i]+GaussianCurve(H0[i],Mean[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>],Sigma[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>],</p><p>Multiplier[<xref ref-type="bibr" rid="scirp.112694-ref4">4</xref>]); } } //End of CreatesFinalGaussianCurve</p><p>//***Returns the Least Mean Square of the equation DA*x^2+DB*x+DC.</p><p>double FindsLMS(double DA, double DB, double DC) {</p><p>int i; /*Dummy index value*/ double LMS = 0; //Least Mean Square</p><p>for(i=PosTipIndex-n;i&lt;=PosTipIndex+n;i++){</p><p>LMS=LMS+Sqr(nbCrossings[i]-(DA*H0[i]*H0[i]+DB*H0[i]+DC));</p><p>} return LMS; } //End of FindsLMS</p><p>//***Returns A, B, and C coefficients of the quadratic equation of the tip</p><p>void ApproximatesTipEquation(void) {</p><p>double LMSTipMin; //Reminds the lowest value of least mean square</p><p>double PLMSTip, NLMSTip; //LMSTip for a forward and backward step</p><p>double DA,DB,DC; //Dummy values of A, B and C coefficients</p><p>double StepA,StepB,StepC; //Step variation of the coefficients</p><p>double nbCrossingsMax = 0; //Maximum number crossings at the tip</p><p>double xa,xb,xc,ya,yb,yc; /*3 coordinates*/ int i; //Dummy index value</p><p>for(i=0;i&lt;=nbH0*2-1;i++) { //Finds the index of the approximated tip</p><p>if (nbCrossings[i]&gt;nbCrossingsMax) {</p><p>nbCrossingsMax=nbCrossings[i]; PosTipIndex=i; } }</p><p>i=PosTipIndex; xa=H0[i-n]; xb=H0[i]; xc=H0[i+n];</p><p>ya=nbCrossings[i-n]; yb=nbCrossings[i]; yc=nbCrossings[i+n];</p><p>//Sets coefficients ABC</p><p>A=((yc-ya)/((xc-xa)*(xc-xb)))-((yb-ya)/((xb-xa)*(xc-xb)));</p><p>B=((yb-ya)/(xb-xa))-A*(xb+xa); C=ya-A*xa*xa-B*xa; DA=A;DB=B;DC=C;</p><p>} //End of ApproximatesTipEquation</p><p>//***Function that returns the Best estimate of H0</p><p>void BestEstimateOfH0(void) {</p><p>CreateTableOfCrossingH0Ranges(); FindsBestGaussiansToFitRealCurve();</p><p>CreatesFinalGaussianCurve(); ApproximatesTipEquation();</p><p>BEH=-B/(2*A); Accuracy_ppm = (BEH-TVH)/(TVH*1E-6);</p><p>LMSTip=FindsLMS(A,B,C); } //End of BesEstimateOfH0</p><p>int main(void) {</p><p>BestEstimateOfH0();</p><p>printf(&quot;\n\n Equation of the tip: y = %.10lfx^2+ %.10lfx+ %.10lf&quot;,A,B,C);</p><p>printf(&quot;\n Best estimate of H0 = %.10lf km/(s*MParsec)&quot;,BEH);</p><p>printf(&quot;\n Theoretical H0 = %.10lf km/(s*MParsec)&quot;,TVH);</p><p>printf(&quot;\n Relative accuracy versus theoretical value = %.10lf ppm&quot;,</p><p>Accuracy_ppm);</p><p>getchar(); return 0;</p><p>} //End of main</p></sec></body><back><ref-list><title>References</title><ref id="scirp.112694-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">Baxter, E.J. and Sherwin, B.D. (2021) Monthly Notices of the Royal Astronomical Society, 501, 1023-1035. https://doi.org/10.1093/mnras/staa3706</mixed-citation></ref><ref id="scirp.112694-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">Blakeslee, J.P., Jensen, J.B., Ma, C.-P., Milne, P.A. and Greene, J.E. (2021) The Astrophysical Journal, 911, Article No. 65. https://doi.org/10.3847/1538-4357/abe86a</mixed-citation></ref><ref id="scirp.112694-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">Bonilla, A., Kumar, S. and Nunes, R.C. (2021) The European Physical Journal C, 81, Article No. 127. https://doi.org/10.1140/epjc/s10052-021-08925-z</mixed-citation></ref><ref id="scirp.112694-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">Dainotti, M.G., et al. (2021) The Astrophysical Journal, 912, Article No. 150. https://doi.org/10.3847/1538-4357/abeb73</mixed-citation></ref><ref id="scirp.112694-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">Denzel, P., Coles, J.P., Saha, P. and Williams, L.L.R. (2021) Monthly Notices of the Royal Astronomical Society, 501, 784-801. https://doi.org/10.1093/mnras/staa3603</mixed-citation></ref><ref id="scirp.112694-ref6"><label>6</label><mixed-citation publication-type="other" xlink:type="simple">Di Valentino, E. (2021) Monthly Notices of the Royal Astronomical Society, 502, 2065-2073. https://doi.org/10.1093/mnras/stab187</mixed-citation></ref><ref id="scirp.112694-ref7"><label>7</label><mixed-citation publication-type="other" xlink:type="simple">Gayathri, V., et al. (2021) The Astrophysical Journal Letters, 908, Article No. L34. https://doi.org/10.3847/2041-8213/abe388</mixed-citation></ref><ref id="scirp.112694-ref8"><label>8</label><mixed-citation publication-type="other" xlink:type="simple">Hagstotz, S., Reischke, R. and Lilow R (2021) A New Measurement of the Hubble Constant Using Fast Radio Bursts. arXiv:2104.04538v1, Not Published.</mixed-citation></ref><ref id="scirp.112694-ref9"><label>9</label><mixed-citation publication-type="other" xlink:type="simple">Khetan, N., et al. (2021) Astronomy and Astrophysics, 647, Article No. A72. https://doi.org/10.1051/0004-6361/202039196</mixed-citation></ref><ref id="scirp.112694-ref10"><label>10</label><mixed-citation publication-type="other" xlink:type="simple">Mukherjee, S., et al. (2021) Astronomy and Astrophysics, 646, Article No. A65. https://doi.org/10.1051/0004-6361/201936724</mixed-citation></ref><ref id="scirp.112694-ref11"><label>11</label><mixed-citation publication-type="other" xlink:type="simple">Park, J.W., et al. (2021) The Astrophysical Journal, 910, Article No. 39. https://doi.org/10.3847/1538-4357/abdfc4</mixed-citation></ref><ref id="scirp.112694-ref12"><label>12</label><mixed-citation publication-type="other" xlink:type="simple">Philcox, O.H.E., Sherwin, B.D., Farren, G.S. and Baxter, E.J. (2021) Physical Review D, 103, Article ID: 023538. https://doi.org/10.1103/PhysRevD.103.023538</mixed-citation></ref><ref id="scirp.112694-ref13"><label>13</label><mixed-citation publication-type="other" xlink:type="simple">Qi, J.-Z., Zhao, J.-W., Cao, S., Biesiada, M. and Liu, Y. (2021) Monthly Notices of the Royal Astronomical Society, 503, 2179-2186. https://doi.org/10.1093/mnras/stab638</mixed-citation></ref><ref id="scirp.112694-ref14"><label>14</label><mixed-citation publication-type="other" xlink:type="simple">Riess, et al. (2021) The Astrophysical Journal Letters, 908, L6. https://doi.org/10.3847/2041-8213/abdbaf</mixed-citation></ref><ref id="scirp.112694-ref15"><label>15</label><mixed-citation publication-type="other" xlink:type="simple">Soltis, J., Casertano, S. and Riess, A.G. (2021) The Astrophysical Journal Letters, 908, L5. https://doi.org/10.3847/2041-8213/abdbad</mixed-citation></ref><ref id="scirp.112694-ref16"><label>16</label><mixed-citation publication-type="other" xlink:type="simple">Wang, H. and Giannios, D. (2021) The Astrophysical Journal, 908, Article No. 200. https://doi.org/10.3847/1538-4357/abd39c</mixed-citation></ref><ref id="scirp.112694-ref17"><label>17</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, J.-C., Jiao, K. and Zhang, T.-J. (2021) Model-Independent meAsurement of the Hubble Constant and the Absolute Magnitude of Type Ia Supernovae. Not Published. arXiv:2101.05897.</mixed-citation></ref><ref id="scirp.112694-ref18"><label>18</label><mixed-citation publication-type="other" xlink:type="simple">Aghanim, N.A., Forveille, T., Pentericci, L. and Shore, S. (2020) Astronomy &amp; Astrophysics, 641, Article No. E1. https://doi.org/10.1051/0004-6361/202039265</mixed-citation></ref><ref id="scirp.112694-ref19"><label>19</label><mixed-citation publication-type="other" xlink:type="simple">Benevento, G., Hu, W. and Raveri, M. (2020) Physical Review D, 101, Article ID: 103517. https://doi.org/10.1103/PhysRevD.101.103517</mixed-citation></ref><ref id="scirp.112694-ref20"><label>20</label><mixed-citation publication-type="other" xlink:type="simple">Birrer, S., et al. (2020) Astronomy &amp; Astrophysics, 643, Article No. A165. https://doi.org/10.1051/0004-6361/202038861</mixed-citation></ref><ref id="scirp.112694-ref21"><label>21</label><mixed-citation publication-type="other" xlink:type="simple">Camarena, D. and Marra, V. (2020) Physical Review Research, 2, Article ID: 013028. https://doi.org/10.1103/PhysRevResearch.2.013028</mixed-citation></ref><ref id="scirp.112694-ref22"><label>22</label><mixed-citation publication-type="other" xlink:type="simple">Chang, Z. and Zhu, Q.-H. (2020) Physical Review D, 101, Article ID: 084029. https://doi.org/10.1103/PhysRevD.101.084029</mixed-citation></ref><ref id="scirp.112694-ref23"><label>23</label><mixed-citation publication-type="other" xlink:type="simple">Coughlin, M.W., et al. (2020) Nature Communications, 11, Article No. 4129. https://doi.org/10.1038/s41467-020-17998-5</mixed-citation></ref><ref id="scirp.112694-ref24"><label>24</label><mixed-citation publication-type="other" xlink:type="simple">D’Agostino, R. and Nunes, R.C. (2020) Physical Review D, 101, Article ID: 103505.https://doi.org/10.1103/PhysRevD.101.103505</mixed-citation></ref><ref id="scirp.112694-ref25"><label>25</label><mixed-citation publication-type="other" xlink:type="simple">Dai, W.M., Ma, Y.-Z. and He, H.-J. (2020) Physical Review D, 102, Article ID: 121302. https://doi.org/10.1103/PhysRevD.102.121302</mixed-citation></ref><ref id="scirp.112694-ref26"><label>26</label><mixed-citation publication-type="other" xlink:type="simple">Wong, K.C., et al. (2017) Monthly Notices of the Royal Astronomical Society, 465, 4895-4913. https://doi.org/10.1093/mnras/stw3077</mixed-citation></ref><ref id="scirp.112694-ref27"><label>27</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, B.R. (2017) Monthly Notices of the Royal Astronomical Society, 471, 2254-2285. https://doi.org/10.1093/mnras/stx1600</mixed-citation></ref><ref id="scirp.112694-ref28"><label>28</label><mixed-citation publication-type="other" xlink:type="simple">Ade, P.A.R., et al. (2016) Astronomy &amp; Astrophysics, 594, Article No. A13. https://doi.org/10.1051/0004-6361/201525830</mixed-citation></ref><ref id="scirp.112694-ref29"><label>29</label><mixed-citation publication-type="other" xlink:type="simple">Gao, F., et al. (2016) The Astrophysical Journal, 817, Article No. 128. https://doi.org/10.3847/0004-637X/817/2/128</mixed-citation></ref><ref id="scirp.112694-ref30"><label>30</label><mixed-citation publication-type="other" xlink:type="simple">Ichiki, K., Yoo, C.-M. and Oguri, M. (2016) Physical Review D, 93, Article ID: 023529. https://doi.org/10.1103/PhysRevD.93.023529</mixed-citation></ref><ref id="scirp.112694-ref31"><label>31</label><mixed-citation publication-type="other" xlink:type="simple">Ludovi&amp;cacute;, V.V., D’Agostino, R. and Vittorio, N. (2016) Astronomy and Astrophysics, 595, Article No. A109. https://doi.org/10.1051/0004-6361/201628217</mixed-citation></ref><ref id="scirp.112694-ref32"><label>32</label><mixed-citation publication-type="other" xlink:type="simple">Moresco, M., et al. (2016) Journal of Cosmology and Astroparticle Physics, 5, Article No. 014. https://doi.org/10.1088/1475-7516/2016/05/014</mixed-citation></ref><ref id="scirp.112694-ref33"><label>33</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (2016) The Astrophysical Journal, 826, Article No. 56. https://doi.org/10.3847/0004-637X/826/1/56</mixed-citation></ref><ref id="scirp.112694-ref34"><label>34</label><mixed-citation publication-type="other" xlink:type="simple">Tully, R.B., Courtois, H.M. and Sorce, J.G. (2016) The Astronomical Journal, 152, Article No. 50. https://doi.org/10.3847/0004-6256/152/2/50</mixed-citation></ref><ref id="scirp.112694-ref35"><label>35</label><mixed-citation publication-type="other" xlink:type="simple">Cheng, C. and Huang, Q.G. (2015) Science China Physics, Mechanics &amp; Astronomy, 58, Article No. 599801. https://doi.org/10.1007/s11433-015-5684-5</mixed-citation></ref><ref id="scirp.112694-ref36"><label>36</label><mixed-citation publication-type="other" xlink:type="simple">Cuesta, A.J., Verde, L., Riess, A. and Jimenez, R. (2015) Monthly Notices of the Royal Astronomical Society, 448, 3463-3471. https://doi.org/10.1093/mnras/stv261</mixed-citation></ref><ref id="scirp.112694-ref37"><label>37</label><mixed-citation publication-type="other" xlink:type="simple">Jang, I.S. and Lee, M.G. (2015) The Astrophysical Journal, 807, Article No. 133. https://doi.org/10.1088/0004-637X/807/2/133</mixed-citation></ref><ref id="scirp.112694-ref38"><label>38</label><mixed-citation publication-type="other" xlink:type="simple">Kumar, S.R., Stalin, C.S. and Prabhu, T.P. (2015) Astronomy and Astrophysics, 580, Article No. A38. https://doi.org/10.1051/0004-6361/201423977</mixed-citation></ref><ref id="scirp.112694-ref39"><label>39</label><mixed-citation publication-type="other" xlink:type="simple">Kuo, C.Y., Braatz, J.A., Lo, K.Y., Reid, M.J., Suyu, S.H., Pesce, D.W., Condon, J.J., Henkel, C. and Impellizzeri, C.M.V. (2015) The Astrophysical Journal, 800, Article No. 26. https://doi.org/10.1088/0004-637X/800/1/26</mixed-citation></ref><ref id="scirp.112694-ref40"><label>40</label><mixed-citation publication-type="other" xlink:type="simple">Rigault, M. and Schombert, J.M. (2015) The Astrophysical Journal, 802, Article No. 18. https://doi.org/10.1088/0004-637X/802/1/18</mixed-citation></ref><ref id="scirp.112694-ref41"><label>41</label><mixed-citation publication-type="other" xlink:type="simple">Ade, P.A.R., et al. (2014) Astronomy &amp; Astrophysics, 571, Article No. A16. https://doi.org/10.1051/0004-6361/201321591</mixed-citation></ref><ref id="scirp.112694-ref42"><label>42</label><mixed-citation publication-type="other" xlink:type="simple">Ben-Dayan, I., Durrer, R., Marozzi, G. and Schwarz, D.J. (2014) Physical Review Letters, 112, Article ID: 221301. https://doi.org/10.1103/PhysRevLett.112.221301</mixed-citation></ref><ref id="scirp.112694-ref43"><label>43</label><mixed-citation publication-type="other" xlink:type="simple">Bennett, C.L., et al. (2014) The Astrophysical Journal, 794, Article No. 135. https://doi.org/10.1088/0004-637X/794/2/135</mixed-citation></ref><ref id="scirp.112694-ref44"><label>44</label><mixed-citation publication-type="other" xlink:type="simple">Busti, V.C., Clarkson, C. and Seikel, M. (2014) Proceedings of the International Astronomical Union, 10, 25-27. https://doi.org/10.1017/S1743921314013751</mixed-citation></ref><ref id="scirp.112694-ref45"><label>45</label><mixed-citation publication-type="other" xlink:type="simple">Efstathiou, G. (2014) Monthly Notices of the Royal Astronomical Society, 440, 1138-1152. https://doi.org/10.1093/mnras/stu278</mixed-citation></ref><ref id="scirp.112694-ref46"><label>46</label><mixed-citation publication-type="other" xlink:type="simple">Lima, J.A.S. and Cunha, J.V. (2014) The Astrophysical Journal Letters, 781, Article No. L38. https://doi.org/10.1088/2041-8205/781/2/L38</mixed-citation></ref><ref id="scirp.112694-ref47"><label>47</label><mixed-citation publication-type="other" xlink:type="simple">Bennett, C.L., et al. (2013) The Astrophysical Journal, 208, Article No. 20.https://doi.org/10.1088/0067-0049/208/2/20</mixed-citation></ref><ref id="scirp.112694-ref48"><label>48</label><mixed-citation publication-type="other" xlink:type="simple">Braatz, J., et al. (2013) Proceedings of the International Astronomical Union, 8, 255-261. https://doi.org/10.1017/S1743921312021515</mixed-citation></ref><ref id="scirp.112694-ref49"><label>49</label><mixed-citation publication-type="other" xlink:type="simple">Farooq, O. and Rathra, B. (2013) The Astrophysical Journal Letters, 766, Article No. L7. https://doi.org/10.1088/2041-8205/766/1/L7</mixed-citation></ref><ref id="scirp.112694-ref50"><label>50</label><mixed-citation publication-type="other" xlink:type="simple">Hinshaw, G., et al. (2013) The Astrophysical Journal Supplement Series, 208, Article No. 19. https://doi.org/10.1088/0067-0049/208/2/19</mixed-citation></ref><ref id="scirp.112694-ref51"><label>51</label><mixed-citation publication-type="other" xlink:type="simple">Humphreys, E.M.L., Reid, M.J., Moran, J.M., Greenhill, L.J. and Argon, A.L. (2013) The Astrophysical Journal, 775, Article No. 13. https://doi.org/10.1088/0004-637X/775/1/13</mixed-citation></ref><ref id="scirp.112694-ref52"><label>52</label><mixed-citation publication-type="other" xlink:type="simple">Kuo, C.Y., Braatz, J.A., Reid, M.J., Lo, K.Y., Condon, J.J., Impellizzeri, C.M.V. and Henkel, C. (2013) The Astrophysical Journal, 767, Article No. 155. https://doi.org/10.1088/0004-637X/767/2/155</mixed-citation></ref><ref id="scirp.112694-ref53"><label>53</label><mixed-citation publication-type="other" xlink:type="simple">Pietrzyński, G., et al. (2013) Nature, 495, 76-79. https://doi.org/10.1038/nature11878</mixed-citation></ref><ref id="scirp.112694-ref54"><label>54</label><mixed-citation publication-type="other" xlink:type="simple">Reid, M.J., et al. (2013) The Astrophysical Journal, 767, Article No. 154.https://doi.org/10.1088/0004-637X/767/2/154</mixed-citation></ref><ref id="scirp.112694-ref55"><label>55</label><mixed-citation publication-type="other" xlink:type="simple">Salvatelli, V., Marchini, A., Lopez-Honorez, L. and Mena, O. (2013) Physical Review D, 88, Article ID: 023531. https://doi.org/10.1103/PhysRevD.88.023531</mixed-citation></ref><ref id="scirp.112694-ref56"><label>56</label><mixed-citation publication-type="other" xlink:type="simple">Scowcroft, V., et al. (2013) Proceedings of the International Astronomical Union, 8, 274-281. https://doi.org/10.1017/S1743921312021540</mixed-citation></ref><ref id="scirp.112694-ref57"><label>57</label><mixed-citation publication-type="other" xlink:type="simple">Sereno, M. and Paraficz, D. (2013) Monthly Notices of the Royal Astronomical Society, 437, 600-605. https://doi.org/10.1093/mnras/stt1938</mixed-citation></ref><ref id="scirp.112694-ref58"><label>58</label><mixed-citation publication-type="other" xlink:type="simple">Wei, J.-J. and Wu, X.-F. (2017) The Astrophysical Journal, 838, Article No. 160. https://doi.org/10.3847/1538-4357/aa674b</mixed-citation></ref><ref id="scirp.112694-ref59"><label>59</label><mixed-citation publication-type="other" xlink:type="simple">Wang, Y., Xu, L. and Zhao, G.-B. (2017) The Astrophysical Journal, 849, Article No. 84. https://doi.org/10.3847/1538-4357/aa8f48</mixed-citation></ref><ref id="scirp.112694-ref60"><label>60</label><mixed-citation publication-type="other" xlink:type="simple">Pritychenko, B. (2017) EPJ Web of Conferences, 146, Article No. 01006. https://doi.org/10.1051/epjconf/201714601006</mixed-citation></ref><ref id="scirp.112694-ref61"><label>61</label><mixed-citation publication-type="other" xlink:type="simple">Jang, I.S. and Lee, M.G. (2017) The Astrophysical Journal, 836, Article No. 74. https://doi.org/10.3847/1538-4357/836/1/74</mixed-citation></ref><ref id="scirp.112694-ref62"><label>62</label><mixed-citation publication-type="other" xlink:type="simple">Huang, H. and Huang, L. (2017) International Journal of Modern Physics D, 26, Article No. 1740001. https://doi.org/10.1142/S0218271817400016</mixed-citation></ref><ref id="scirp.112694-ref63"><label>63</label><mixed-citation publication-type="other" xlink:type="simple">Hjorth, J., et al. (2017) The Astrophysical Journal Letters, 848, Article No. L31. https://doi.org/10.3847/2041-8213/aa9110</mixed-citation></ref><ref id="scirp.112694-ref64"><label>64</label><mixed-citation publication-type="other" xlink:type="simple">Guo, R.-Y. and Zhang, X. (2017) The European Physical Journal C, 77, Article No. 882. https://doi.org/10.1140/epjc/s10052-017-5454-9</mixed-citation></ref><ref id="scirp.112694-ref65"><label>65</label><mixed-citation publication-type="other" xlink:type="simple">Grieb, J.N., et al. (2017) Monthly Notices of the Royal Astronomical Society, 467, 2085-2112. https://doi.org/10.1093/mnras/stw3384</mixed-citation></ref><ref id="scirp.112694-ref66"><label>66</label><mixed-citation publication-type="other" xlink:type="simple">Feeney, S.M., Mortlock, D.J. and Dalmasso, N. (2017) Monthly Notices of the Royal Astronomical Society, 476, 3861-3882. https://doi.org/10.1093/mnras/sty418</mixed-citation></ref><ref id="scirp.112694-ref67"><label>67</label><mixed-citation publication-type="other" xlink:type="simple">Farooq, O., Madiyar, F.R., Crandall, S. and Ratra, B. (2017) The Astrophysical Journal, 835, Article No. 26. https://doi.org/10.3847/1538-4357/835/1/26</mixed-citation></ref><ref id="scirp.112694-ref68"><label>68</label><mixed-citation publication-type="other" xlink:type="simple">Chen, Y., Kumar, S. and Ratra, B. (2017) The Astrophysical Journal, 835, Article No. 86. https://doi.org/10.3847/1538-4357/835/1/86</mixed-citation></ref><ref id="scirp.112694-ref69"><label>69</label><mixed-citation publication-type="other" xlink:type="simple">Cardona, W., Kunza, M. and Valeria, P. (2017) Journal of Cosmology and Astroparticle Physics, 3, Article No. 056. https://doi.org/10.1088/1475-7516/2017/03/056</mixed-citation></ref><ref id="scirp.112694-ref70"><label>70</label><mixed-citation publication-type="other" xlink:type="simple">Bonvin, V., et al. (2017) Monthly Notices of the Royal Astronomical Society, 465, 4914-4930. https://doi.org/10.1093/mnras/stw3006</mixed-citation></ref><ref id="scirp.112694-ref71"><label>71</label><mixed-citation publication-type="other" xlink:type="simple">Bethapudi, S. and Desai, S. (2017) The European Physical Journal Plus, 132, Article No. 78. https://doi.org/10.1140/epjp/i2017-11390-3</mixed-citation></ref><ref id="scirp.112694-ref72"><label>72</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, B.P., et al. (2017) Nature, 551, 85-88. https://doi.org/10.1038/nature24471</mixed-citation></ref><ref id="scirp.112694-ref73"><label>73</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, J. (2018) Publications of the Astronomical Society of the Pacific, 130, Article ID: 117002. https://doi.org/10.1088/1538-3873/aae4ca</mixed-citation></ref><ref id="scirp.112694-ref74"><label>74</label><mixed-citation publication-type="other" xlink:type="simple">Yu, H., Ratra, B. and Wang, F.-Y. (2018) The Astrophysical Journal, 856, Article No. 3. https://doi.org/10.3847/1538-4357/aab0a2</mixed-citation></ref><ref id="scirp.112694-ref75"><label>75</label><mixed-citation publication-type="other" xlink:type="simple">Vitale, S. and Chen, H.-Y. (2018) Physical Review Letters, 121, Article ID: 021303. https://doi.org/10.1103/PhysRevLett.121.021303</mixed-citation></ref><ref id="scirp.112694-ref76"><label>76</label><mixed-citation publication-type="other" xlink:type="simple">Van Putten, M.H.P.M. (2018) European Physical Journal Web of Conferences, 168, Article No. 08005. https://doi.org/10.1051/epjconf/201816808005</mixed-citation></ref><ref id="scirp.112694-ref77"><label>77</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (2018) The Astrophysical Journal, 855, Article No. 136.</mixed-citation></ref><ref id="scirp.112694-ref78"><label>78</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (2018) The Astrophysical Journal, 861, 1-13.</mixed-citation></ref><ref id="scirp.112694-ref79"><label>79</label><mixed-citation publication-type="book" xlink:type="simple">Lee, M.G. and Jang, I.S. (2018) The TRGB and the Hubble Constant in 2017: TIPSNU. In: Jensen, J., Michael Rich, R. and de Grijs, R., Eds., Stellar Populations and the Distance Scale, Vol. 514, Astronomical Society of the Pacific, San Francisco, 143-150.</mixed-citation></ref><ref id="scirp.112694-ref80"><label>80</label><mixed-citation publication-type="other" xlink:type="simple">Hoeneisen, B. (2018) International Journal of Astronomy and Astrophysics, 8, 386-405. https://doi.org/10.4236/ijaa.2018.84027</mixed-citation></ref><ref id="scirp.112694-ref81"><label>81</label><mixed-citation publication-type="other" xlink:type="simple">Grillo, C., et al. (2018) The Astrophysical Journal, 860, Article No. 94. https://doi.org/10.3847/1538-4357/aac2c9</mixed-citation></ref><ref id="scirp.112694-ref82"><label>82</label><mixed-citation publication-type="other" xlink:type="simple">Gómez-Valent, A. and Amendola, L. (2018) Journal of Cosmology and Astroparticle Physics, 4, Article No. 051. https://doi.org/10.1088/1475-7516/2018/04/051</mixed-citation></ref><ref id="scirp.112694-ref83"><label>83</label><mixed-citation publication-type="other" xlink:type="simple">Di Valentino, E. and Melchiorri, A. (2018) Physical Review D, 97, Article ID: 041301. https://doi.org/10.1103/PhysRevD.97.041301</mixed-citation></ref><ref id="scirp.112694-ref84"><label>84</label><mixed-citation publication-type="other" xlink:type="simple">Dhawan, S., Jha, S.W. and Leibundgut, B. (2018) Astronomy and Astrophysics, 609, Article No. A72. https://doi.org/10.1051/0004-6361/201731501</mixed-citation></ref><ref id="scirp.112694-ref85"><label>85</label><mixed-citation publication-type="other" xlink:type="simple">Choudhury, S.R. and Choubey, S. (2019) Journal of Cosmology and Astroparticle Physics, 9, Article No. 017. https://doi.org/10.1088/1475-7516/2018/09/017</mixed-citation></ref><ref id="scirp.112694-ref86"><label>86</label><mixed-citation publication-type="other" xlink:type="simple">Chen, H.-Y., Fishbach, M. and Holz, D.E. (2018) Nature, 562, 545-547. https://doi.org/10.1038/s41586-018-0606-0</mixed-citation></ref><ref id="scirp.112694-ref87"><label>87</label><mixed-citation publication-type="other" xlink:type="simple">Cantiello, M., et al. (2018) The Astrophysical Journal Letters, 854, Article No. L31.https://doi.org/10.3847/2041-8213/aaad64</mixed-citation></ref><ref id="scirp.112694-ref88"><label>88</label><mixed-citation publication-type="other" xlink:type="simple">Braatz, J., et al. (2018) Proceedings of the International Astronomical Union, 13, 86-91. https://doi.org/10.1017/S1743921317010249</mixed-citation></ref><ref id="scirp.112694-ref89"><label>89</label><mixed-citation publication-type="other" xlink:type="simple">Bolejko, K. (2018) Physical Review D, 97, Article ID: 083515. https://doi.org/10.1103/PhysRevD.97.083515</mixed-citation></ref><ref id="scirp.112694-ref90"><label>90</label><mixed-citation publication-type="other" xlink:type="simple">Benetti, M., Graef, L.L. and Alcaniz, J.S. (2018) Journal of Cosmology and Astroparticle Physics, 7, Article No. 066. https://doi.org/10.1088/1475-7516/2018/07/066</mixed-citation></ref><ref id="scirp.112694-ref91"><label>91</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, T.M.C., et al. (2018) Monthly Notices of the Royal Astronomical Society, 480, 3879-3888. https://doi.org/10.1093/mnras/sty1939</mixed-citation></ref><ref id="scirp.112694-ref92"><label>92</label><mixed-citation publication-type="other" xlink:type="simple">Zeng, H. and Yan, D. (2019) The Astrophysical Journal, 882, Article No. 87. https://doi.org/10.3847/1538-4357/ab35e3</mixed-citation></ref><ref id="scirp.112694-ref93"><label>93</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, X. and Huang, Q.-G. (2019) Communications in Theoretical Physics, 71, 826-830. https://doi.org/10.1088/0253-6102/71/7/826</mixed-citation></ref><ref id="scirp.112694-ref94"><label>94</label><mixed-citation publication-type="other" xlink:type="simple">Yuan, W., et al. (2019) The Astrophysical Journal, 886, Article No. 61. https://doi.org/10.3847/1538-4357/ab4bc9</mixed-citation></ref><ref id="scirp.112694-ref95"><label>95</label><mixed-citation publication-type="other" xlink:type="simple">Wong, K.C., et al. (2019) Monthly Notices of the Royal Astronomical Society, 498, 1420-1439. https://doi.org/10.1093/mnras/stz3094</mixed-citation></ref><ref id="scirp.112694-ref96"><label>96</label><mixed-citation publication-type="other" xlink:type="simple">Verde, L., Treu, T. and Riess, A.G. (2019) Nature Astronomy, 3, 891-895. https://doi.org/10.1038/s41550-019-0902-0</mixed-citation></ref><ref id="scirp.112694-ref97"><label>97</label><mixed-citation publication-type="other" xlink:type="simple">Tiwari, S., Haney, M. and Boetzel, Y. (2019) A Gravitational-Wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo. University of Zurich, Zurich, Not Published. arXiv.org 1908.06060.</mixed-citation></ref><ref id="scirp.112694-ref98"><label>98</label><mixed-citation publication-type="other" xlink:type="simple">Taubenberger, S., et al. (2019) Astronomy and Astrophysics, 628, Article No. L7. https://doi.org/10.1051/0004-6361/201935980</mixed-citation></ref><ref id="scirp.112694-ref99"><label>99</label><mixed-citation publication-type="other" xlink:type="simple">Soares-Santos, M., et al. (2019) The Astrophysical Journal Letters, 876, Article No. L7. https://doi.org/10.3847/2041-8213/ab14f1</mixed-citation></ref><ref id="scirp.112694-ref100"><label>100</label><mixed-citation publication-type="other" xlink:type="simple">Shajib, A.J., Birrer, S., Treu, T., Agnello, A., et al. (2019) Monthly Notices of the Royal Astronomical Society, 494, 6072-6102. https://doi.org/10.1093/mnras/staa828</mixed-citation></ref><ref id="scirp.112694-ref101"><label>101</label><mixed-citation publication-type="other" xlink:type="simple">Saha, S. and Sahoo, S. (2019) The African Review of Physics, 14, 7-9.</mixed-citation></ref><ref id="scirp.112694-ref102"><label>102</label><mixed-citation publication-type="other" xlink:type="simple">Ryan, J., Chen, Y. and Ratra, B. (2019) Monthly Notices of the Royal Astronomical Society, 488, 3844-3856. https://doi.org/10.1093/mnras/stz1966</mixed-citation></ref><ref id="scirp.112694-ref103"><label>103</label><mixed-citation publication-type="other" xlink:type="simple">Rusu, C.E., et al. (2020) Monthly Notices of the Royal Astronomical Society, 498, 1440-1468. https://doi.org/10.1093/mnras/stz3451</mixed-citation></ref><ref id="scirp.112694-ref104"><label>104</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G. (2019) Nature Reviews Physics, 2, 10-12. https://doi.org/10.1038/s42254-019-0137-0</mixed-citation></ref><ref id="scirp.112694-ref105"><label>105</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (2019) The Astrophysical Journal, 876, Article No. 85. https://doi.org/10.3847/1538-4357/ab1422</mixed-citation></ref><ref id="scirp.112694-ref106"><label>106</label><mixed-citation publication-type="other" xlink:type="simple">Reid, M.J., Pesce, D.W. and Riess, A.G. (2019) The Astrophysical Journal, 886, Article No. L27. https://doi.org/10.3847/2041-8213/ab552d</mixed-citation></ref><ref id="scirp.112694-ref107"><label>107</label><mixed-citation publication-type="other" xlink:type="simple">Park, C.-G. and Ratra, B. (2019) Astrophysics and Space Science, 364, Article No. 134. https://doi.org/10.1007/s10509-019-3627-8</mixed-citation></ref><ref id="scirp.112694-ref108"><label>108</label><mixed-citation publication-type="other" xlink:type="simple">Martinelli, M. and Tutusaus, I. (2019) Symmetry, 11, Article No. 986. https://doi.org/10.3390/sym11080986</mixed-citation></ref><ref id="scirp.112694-ref109"><label>109</label><mixed-citation publication-type="other" xlink:type="simple">Macaulay, E., et al. (2019) Monthly Notices of the Royal Astronomical Society, 486, 2184-2196. https://doi.org/10.1093/mnras/stz978</mixed-citation></ref><ref id="scirp.112694-ref110"><label>110</label><mixed-citation publication-type="other" xlink:type="simple">Liao, K., Shafieloo, A., Keeley, R.E. and Linder, E.V. (2019) The Astrophysical Journal Letters, 886, Article No. L23. https://doi.org/10.3847/2041-8213/ab5308</mixed-citation></ref><ref id="scirp.112694-ref111"><label>111</label><mixed-citation publication-type="other" xlink:type="simple">Kozmanyan, A., Bourdin, H., Mazzotta, P., Rasia, E. and Sereno, M. (2019) Astronomy &amp; Astrophysics, 621, Article No. A34. https://doi.org/10.1051/0004-6361/201833879</mixed-citation></ref><ref id="scirp.112694-ref112"><label>112</label><mixed-citation publication-type="other" xlink:type="simple">Jee, I., et al. (2019) Science, 365, 1134-1138. https://doi.org/10.1126/science.aat7371</mixed-citation></ref><ref id="scirp.112694-ref113"><label>113</label><mixed-citation publication-type="other" xlink:type="simple">Hotokezaka, K., et al. (2019) Nature Astronomy, 3, 940-944. https://doi.org/10.1038/s41550-019-0820-1</mixed-citation></ref><ref id="scirp.112694-ref114"><label>114</label><mixed-citation publication-type="other" xlink:type="simple">Guo, R.-Y., Zhang, J.-F. and Zhang, X. (2019) Journal of Cosmology and Astroparticle Physics, 2, Article No. 054. https://doi.org/10.1088/1475-7516/2019/02/054</mixed-citation></ref><ref id="scirp.112694-ref115"><label>115</label><mixed-citation publication-type="other" xlink:type="simple">Freedman, W.L., et al. (2019) The Astrophysical Journal, 882, Article No. 34. https://doi.org/10.3847/1538-4357/ab2f73</mixed-citation></ref><ref id="scirp.112694-ref116"><label>116</label><mixed-citation publication-type="other" xlink:type="simple">Fishbach, M., et al. (2019) The Astrophysical Journal Letters, 871, Article No. L13. https://doi.org/10.3847/2041-8213/aaf96e</mixed-citation></ref><ref id="scirp.112694-ref117"><label>117</label><mixed-citation publication-type="other" xlink:type="simple">Dutta, K., et al. (2019) Physical Review D, 100, Article ID: 075028. https://doi.org/10.1103/PhysRevD.100.075028</mixed-citation></ref><ref id="scirp.112694-ref118"><label>118</label><mixed-citation publication-type="other" xlink:type="simple">Domínguez, A., et al. (2019) The Astrophysical Journal, 885, Article No. 137. https://doi.org/10.3847/1538-4357/ab4a0e</mixed-citation></ref><ref id="scirp.112694-ref119"><label>119</label><mixed-citation publication-type="other" xlink:type="simple">Cuceu, A., Farr, J., Lemos, P. and Font-Ribera, A. (2019) Journal of Cosmology and Astroparticle Physics, 10, Article No. 044. https://doi.org/10.1088/1475-7516/2019/10/044</mixed-citation></ref><ref id="scirp.112694-ref120"><label>120</label><mixed-citation publication-type="other" xlink:type="simple">Collett, T., Montanari, F. and R&amp;auml;s&amp;auml;nen, S. (2019) Physical Review Letters, 123, Article ID: 231101. https://doi.org/10.1103/PhysRevLett.123.231101</mixed-citation></ref><ref id="scirp.112694-ref121"><label>121</label><mixed-citation publication-type="other" xlink:type="simple">Chen, G.C.-F., Fassnacht, C.D., Suyu, S.H., Rusu CE, et al. (2019) Monthly Notices of the Royal Astronomical Society, 490, 1743-1773. https://doi.org/10.1093/mnras/stz2547</mixed-citation></ref><ref id="scirp.112694-ref122"><label>122</label><mixed-citation publication-type="other" xlink:type="simple">Chang, Z., Huang, Q.-G., Wang, S. and Zhao, Z.-C. (2019) The European Physical Journal C, 79, Article No. 177. https://doi.org/10.1140/epjc/s10052-019-6664-0</mixed-citation></ref><ref id="scirp.112694-ref123"><label>123</label><mixed-citation publication-type="other" xlink:type="simple">Birrer, S., Treu, T., Rusu, C.E., Bonvin, V., et al. (2019) Monthly Notices of the Royal Astronomical Society, 484, 4726-4753. https://doi.org/10.1093/mnras/stz200</mixed-citation></ref><ref id="scirp.112694-ref124"><label>124</label><mixed-citation publication-type="other" xlink:type="simple">Anderson, R.I. (2019) Astronomy &amp; Astrophysics, 631, Article No. A165. https://doi.org/10.1051/0004-6361/201936585</mixed-citation></ref><ref id="scirp.112694-ref125"><label>125</label><mixed-citation publication-type="other" xlink:type="simple">Agrawal, P., Cyr-Racine, F.-Y., Pinner, D. and Randall, L. (2019) Rock ‘n’ Roll Solutions to the Hubble Tension. Cornell University, Ithaca, arXiv:1904.01016v1, Not Published.</mixed-citation></ref><ref id="scirp.112694-ref126"><label>126</label><mixed-citation publication-type="other" xlink:type="simple">Zhang, X. and Huang, Q.-G. (2020) Science China Physics Mechanical Astronomy, 63, Article No. 290402. https://doi.org/10.1007/s11433-019-1504-8</mixed-citation></ref><ref id="scirp.112694-ref127"><label>127</label><mixed-citation publication-type="other" xlink:type="simple">Yang, T., Birrer, S. and Hu, B. (2020) Monthly Notices of the Royal Astronomical Society, 497, L56-L61. https://doi.org/10.1093/mnrasl/slaa107</mixed-citation></ref><ref id="scirp.112694-ref128"><label>128</label><mixed-citation publication-type="other" xlink:type="simple">Wu, W.L.K., Motloch, P., Hu, W. and Raveri, M. (2020) Physical Review D, 102, Article ID: 023510. https://doi.org/10.1103/PhysRevD.102.023510</mixed-citation></ref><ref id="scirp.112694-ref129"><label>129</label><mixed-citation publication-type="other" xlink:type="simple">Wei, J.-J. and Melia, F. (2020) The Astrophysical Journal, 897, Article No. 127.https://doi.org/10.3847/1538-4357/ab959b</mixed-citation></ref><ref id="scirp.112694-ref130"><label>130</label><mixed-citation publication-type="other" xlink:type="simple">Vogl, V. (2020) Cosmological Distances of Type II Supernovae from Radiative Transfer Modeling. Dissertation, Max-Planck-Institut Fur Astrophysik, Garching bei München, 172 p, Not Published. https://mediatum.ub.tum.de/doc/1542626/1542626.pdf</mixed-citation></ref><ref id="scirp.112694-ref131"><label>131</label><mixed-citation publication-type="other" xlink:type="simple">Vasylyev, S.S. and Filippenko, A.V. (2020) The Astrophysical Journal, 902, Article No. 149. https://doi.org/10.3847/1538-4357/abb5f9</mixed-citation></ref><ref id="scirp.112694-ref132"><label>132</label><mixed-citation publication-type="other" xlink:type="simple">Sharov, G.S. and Sinyakov, E.S. (2020) Mathematical Modelling and Geometry, 8, 1-20. https://doi.org/10.26456/mmg/2020-811</mixed-citation></ref><ref id="scirp.112694-ref133"><label>133</label><mixed-citation publication-type="other" xlink:type="simple">Shajib, A.J., et al. (2020) Monthly Notices of the Royal Astronomical Society, 494, 6072-6102. https://doi.org/10.1093/mnras/staa828</mixed-citation></ref><ref id="scirp.112694-ref134"><label>134</label><mixed-citation publication-type="other" xlink:type="simple">Schombert, J., McGaugh, S. and Lelli, F. (2020) The Astronomical Journal, 160, Article No. 71. https://doi.org/10.3847/1538-3881/ab9d88</mixed-citation></ref><ref id="scirp.112694-ref135"><label>135</label><mixed-citation publication-type="other" xlink:type="simple">Guo, R.-Y., Zhang, J.-F. and Zhang, X. (2020) Science China Physics, Mechanics &amp; Astronomy, 63, Article No. 290406. https://doi.org/10.1007/s11433-019-1514-0</mixed-citation></ref><ref id="scirp.112694-ref136"><label>136</label><mixed-citation publication-type="other" xlink:type="simple">Pogosian, L., Zhao, G.-B. and Jedamzik, K. (2020) The Astrophysical Journal Letters, 904, Article No. L17. https://doi.org/10.3847/2041-8213/abc6a8</mixed-citation></ref><ref id="scirp.112694-ref137"><label>137</label><mixed-citation publication-type="other" xlink:type="simple">Pesce, D.W., Braatz, J.A., Reid, M.J., Riess, A.G., et al. (2020) The Astrophysical Journal, 891, Article No. L1. https://doi.org/10.3847/2041-8213/ab75f0</mixed-citation></ref><ref id="scirp.112694-ref138"><label>138</label><mixed-citation publication-type="other" xlink:type="simple">Pandey, K.L., Karwalb, T. and Dasc, S. (2020) Journal of Cosmology and Astroparticle Physics, 7, Article No. 026. https://doi.org/10.1088/1475-7516/2020/01/026</mixed-citation></ref><ref id="scirp.112694-ref139"><label>139</label><mixed-citation publication-type="other" xlink:type="simple">Palmese, A., et al. (2020) The Astrophysical Journal Letters, 900, Article No. L33. https://doi.org/10.3847/2041-8213/abaeff</mixed-citation></ref><ref id="scirp.112694-ref140"><label>140</label><mixed-citation publication-type="other" xlink:type="simple">Niedermann, F. and Sloth, M.S. (2020) Physical Review D, 102, Article ID: 063527. https://doi.org/10.1103/PhysRevD.102.063527</mixed-citation></ref><ref id="scirp.112694-ref141"><label>141</label><mixed-citation publication-type="other" xlink:type="simple">Nicolaou, C., Lahav, O., Lemos, P., Hartley, W. and Braden, J. (2020) Monthly Notices of the Royal Astronomical Society, 495, 90-97. https://doi.org/10.1093/mnras/staa1120</mixed-citation></ref><ref id="scirp.112694-ref142"><label>142</label><mixed-citation publication-type="other" xlink:type="simple">Mukherjee, S., Ghosh, A., Graham, M.J., Karathanasis, C., et al. (2020) First Measurement of the Hubble Parameter from Bright Binary Black Hole GW190521. Not Published (Under Review with MNRAS), arXiv:2009.14199, 1 8.</mixed-citation></ref><ref id="scirp.112694-ref143"><label>143</label><mixed-citation publication-type="other" xlink:type="simple">Millon, M., et al. (2020) Astronomy and Astrophysics, 639, Article No. A101. https://doi.org/10.1051/0004-6361/201937351</mixed-citation></ref><ref id="scirp.112694-ref144"><label>144</label><mixed-citation publication-type="other" xlink:type="simple">Lombriser, L. (2020) Physics Letters B, 803, Arrticle ID: 135303. https://doi.org/10.1016/j.physletb.2020.135303</mixed-citation></ref><ref id="scirp.112694-ref145"><label>145</label><mixed-citation publication-type="other" xlink:type="simple">Li, H. and Zhang, X. (2020) Science Bulletin, 65, 1419-1421. https://doi.org/10.1016/j.scib.2020.04.038</mixed-citation></ref><ref id="scirp.112694-ref146"><label>146</label><mixed-citation publication-type="other" xlink:type="simple">Kreisch, C.D., Cyr-Racine, F.-Y. and Doré, O. (2020) Physical Review D, 101, Arrticle ID: 123505. https://doi.org/10.1103/PhysRevD.101.123505</mixed-citation></ref><ref id="scirp.112694-ref147"><label>147</label><mixed-citation publication-type="other" xlink:type="simple">Kim, Y.J., Kang, J., Lee, M.G. and Jang, I.S. (2020) The Astrophysical Journal, 905, Article No. 104. https://doi.org/10.3847/1538-4357/abbd97</mixed-citation></ref><ref id="scirp.112694-ref148"><label>148</label><mixed-citation publication-type="other" xlink:type="simple">De Jaeger, T., Stahl, B.E., Zheng, W., Filippenko, A.V., Riess, A.G. and Galbany, L. (2020) Monthly Notices of the Royal Astronomical Society, 496, 3402–3411. https://doi.org/10.1093/mnras/staa1801</mixed-citation></ref><ref id="scirp.112694-ref149"><label>149</label><mixed-citation publication-type="other" xlink:type="simple">Howlett, C. and Davis, T.M. (2020) Monthly Notices of the Royal Astronomical Society, 492, 3803-3815. https://doi.org/10.1093/mnras/staa049</mixed-citation></ref><ref id="scirp.112694-ref150"><label>150</label><mixed-citation publication-type="other" xlink:type="simple">Holanda, R.F.L., Pordeus-da-Silva, G. and Pereira, S.H. (2020) Journal of Cosmology and Astroparticle Physics, 9, Article No. 053. https://doi.org/10.1088/1475-7516/2020/09/053</mixed-citation></ref><ref id="scirp.112694-ref151"><label>151</label><mixed-citation publication-type="other" xlink:type="simple">Harvey, D. (2020) Monthly Notices of the Royal Astronomical Society, 498, 2871-2886. https://doi.org/10.1093/mnras/staa2522</mixed-citation></ref><ref id="scirp.112694-ref152"><label>152</label><mixed-citation publication-type="other" xlink:type="simple">Haboury, N. (2020) Measuring the Hubble Constant with Standard Sirens. University of Geneva, Astronomy Department, Geneva, 1-22, Not Published. https://www.researchgate.net/publication/343679057_Measuring_the_Hubble_constant_with_standard_sirens</mixed-citation></ref><ref id="scirp.112694-ref153"><label>153</label><mixed-citation publication-type="other" xlink:type="simple">González-Serrena, B., Cuesta, A.J. and Ortiz-Mora, A. (2020) Contributions to the XIV.0 Scientific Meeting (Virtual) of the Spanish Astronomical Society.</mixed-citation></ref><ref id="scirp.112694-ref154"><label>154</label><mixed-citation publication-type="other" xlink:type="simple">Gonzalez, M., Hertzberg, M.P. and Rompineve, F. (2020) Journal of Cosmology and Astroparticle Physics, 10, Article No. 028. https://doi.org/10.1088/1475-7516/2020/10/028</mixed-citation></ref><ref id="scirp.112694-ref155"><label>155</label><mixed-citation publication-type="other" xlink:type="simple">Dietrich, T., et al. (2020) Science, 370, 1450-1453. https://doi.org/10.1126/science.abb4317</mixed-citation></ref><ref id="scirp.112694-ref156"><label>156</label><mixed-citation publication-type="other" xlink:type="simple">Addison, G.E. (2021) The Astrophysical Journal, 912, Article No. L1. https://doi.org/10.3847/2041-8213/abf56e</mixed-citation></ref><ref id="scirp.112694-ref157"><label>157</label><mixed-citation publication-type="other" xlink:type="simple">Abbott, B.P., et al. (2021) The Astrophysical Journal, 909, Article No. 218. https://doi.org/10.3847/1538-4357/abdcb7</mixed-citation></ref><ref id="scirp.112694-ref158"><label>158</label><mixed-citation publication-type="other" xlink:type="simple">Kimura, K., Hashimoto, M., Sakoda, K. and Sakoda, K. (2001) The Astrophysical Journal, 561, L19-L22. https://doi.org/10.1086/324569</mixed-citation></ref><ref id="scirp.112694-ref159"><label>159</label><mixed-citation publication-type="other" xlink:type="simple">Mercier, C. (2016) More than a Hundred Ways to Get the Large Number N. Not Published. http://pragtec.com/physique/index_en.html</mixed-citation></ref><ref id="scirp.112694-ref160"><label>160</label><mixed-citation publication-type="other" xlink:type="simple">Partridge, R.B. (1997) An Introduction to the Cosmic Microwave Background Radiation. From Quantum Fluctuations to Cosmological Structures: Proceedings of the 1st Moroccan School of Astrophysics, Casablanca, 1-10 December 1996, 141-184.</mixed-citation></ref><ref id="scirp.112694-ref161"><label>161</label><mixed-citation publication-type="other" xlink:type="simple">Gush, H.P. (1981) Physical Review Letters, 47, 745-748. https://doi.org/10.1103/PhysRevLett.47.745</mixed-citation></ref><ref id="scirp.112694-ref162"><label>162</label><mixed-citation publication-type="other" xlink:type="simple">Dirac, P.A.M. (1974) Proceedings of the Royal Society of London A: Mathematical, Physical and Engineering Sciences, 338, 439-446. https://doi.org/10.1098/rspa.1974.0095</mixed-citation></ref><ref id="scirp.112694-ref163"><label>163</label><mixed-citation publication-type="other" xlink:type="simple">Dirac, P.A.M. (1938) Proceedings of the Royal Society of London A: Mathematical, Physical and Engineering Sciences, 165, 199-208. https://doi.org/10.1098/rspa.1938.0053</mixed-citation></ref><ref id="scirp.112694-ref164"><label>164</label><mixed-citation publication-type="other" xlink:type="simple">Carvalho, J.C. (1995) International Journal of Theoretical Physics, 34, 2507-2509. https://doi.org/10.1007/BF00670782</mixed-citation></ref><ref id="scirp.112694-ref165"><label>165</label><mixed-citation publication-type="other" xlink:type="simple">Zichichi, A. (2000) Proceedings of the International School of Subnuclear Physics, 36, 1-708.</mixed-citation></ref><ref id="scirp.112694-ref166"><label>166</label><mixed-citation publication-type="other" xlink:type="simple">Mercier, C. (2019) Journal of Modern Physics, 10, 980-1001. https://doi.org/10.4236/jmp.2019.108065</mixed-citation></ref><ref id="scirp.112694-ref167"><label>167</label><mixed-citation publication-type="other" xlink:type="simple">Mulligan, J.F. (1976) American Journal of Physics, 44, 960-969. https://doi.org/10.1119/1.10241</mixed-citation></ref><ref id="scirp.112694-ref168"><label>168</label><mixed-citation publication-type="other" xlink:type="simple">Binney, J. and Merrifield, M. (1998) Galactic Astronomy. Princeton University Press, Princeton, 816 p. https://press.princeton.edu/titles/6358.html</mixed-citation></ref><ref id="scirp.112694-ref169"><label>169</label><mixed-citation publication-type="other" xlink:type="simple">Gr&amp;oslash;n, &amp;Oslash;. (2016) American Journal of Physics, 84, 537-541. https://doi.org/10.1119/1.4944031</mixed-citation></ref><ref id="scirp.112694-ref170"><label>170</label><mixed-citation publication-type="other" xlink:type="simple">Einstein, A. (1911) Annalen der Physik, 340, 898-908. https://doi.org/10.1002/andp.19113401005</mixed-citation></ref><ref id="scirp.112694-ref171"><label>171</label><mixed-citation publication-type="other" xlink:type="simple">Einstein, A. (1905) Annalen der Physik, 322, 891-921. https://doi.org/10.1002/andp.19053221004</mixed-citation></ref><ref id="scirp.112694-ref172"><label>172</label><mixed-citation publication-type="other" xlink:type="simple">Jenkins, A., Villard, R. and Riess, A (2018) Hubblesite.https://stsci-opo.org/STScI-01EVSQXZ976ZY1QKQX17XJ7P5H.pdf</mixed-citation></ref><ref id="scirp.112694-ref173"><label>173</label><mixed-citation publication-type="other" xlink:type="simple">Mohr, P.J., Newell, D.B. and Taylor, B.N. (2016) Review of Modern Physics, 88, Article ID: 035009. https://doi.org/10.1103/RevModPhys.88.035009</mixed-citation></ref><ref id="scirp.112694-ref174"><label>174</label><mixed-citation publication-type="other" xlink:type="simple">Mercier, C. (2020) Journal of Modern Physics, 11, 1428-1465. https://doi.org/10.4236/jmp.2020.119089</mixed-citation></ref><ref id="scirp.112694-ref175"><label>175</label><mixed-citation publication-type="other" xlink:type="simple">Mercier, C. (2019) Journal of Modern Physics, 10, 641-662. https://doi.org/10.4236/jmp.2019.106046</mixed-citation></ref><ref id="scirp.112694-ref176"><label>176</label><mixed-citation publication-type="other" xlink:type="simple">Verde, L., Treu, T. and Riess, A.G. (2019) Nature Astronomy, 3, 891-895. https://doi.org/10.1038/s41550-019-0902-0</mixed-citation></ref><ref id="scirp.112694-ref177"><label>177</label><mixed-citation publication-type="journal" xlink:type="simple"><name name-style="western"><surname>Lema&amp;icirc;tre</surname><given-names> G. </given-names></name>,<etal>et al</etal>. (<year>1927</year>)<article-title>Annales de la Société Scientifique de Bruxelles, A47, 49-59</article-title><source> Partially Translated in English: (1931) Monthly Notices of the Royal Astronomical Society</source><volume> 91</volume>,<fpage> 483</fpage>-<lpage>490</lpage>.<pub-id pub-id-type="doi"></pub-id></mixed-citation></ref><ref id="scirp.112694-ref178"><label>178</label><mixed-citation publication-type="other" xlink:type="simple">Friedman, A. (1922) Zeitschrift für Physics, 10, 377-386. https://doi.org/10.1007/BF01332580</mixed-citation></ref><ref id="scirp.112694-ref179"><label>179</label><mixed-citation publication-type="other" xlink:type="simple">Einstein, A. (1916) Annalen der Physik, 354, 769-822. https://doi.org/10.1002/andp.19163540702</mixed-citation></ref><ref id="scirp.112694-ref180"><label>180</label><mixed-citation publication-type="other" xlink:type="simple">Hubble, E. (1929) Proceedings of the National Academy of Sciences of the United States of America, 15, 168-1973. https://doi.org/10.1073/pnas.15.3.168</mixed-citation></ref><ref id="scirp.112694-ref181"><label>181</label><mixed-citation publication-type="other" xlink:type="simple">Suyu, S.H., et al. (2013) The Astrophysical Journal, 766, Article No. 70. https://doi.org/10.1088/0004-637X/766/2/70</mixed-citation></ref><ref id="scirp.112694-ref182"><label>182</label><mixed-citation publication-type="other" xlink:type="simple">Tully, R.B., et al. (2013) The Astronomical Journal, 146, Article No. 86. https://doi.org/10.1088/0004-6256/146/4/86</mixed-citation></ref><ref id="scirp.112694-ref183"><label>183</label><mixed-citation publication-type="other" xlink:type="simple">Xia, J.-Q., Li, H. and Zhang, X. (2013) Physical Review D, 88, Article ID: 063501. https://doi.org/10.1103/PhysRevD.88.063501</mixed-citation></ref><ref id="scirp.112694-ref184"><label>184</label><mixed-citation publication-type="other" xlink:type="simple">Calabrese, E., Archidiacono, M., Melchiorri, A. and Ratra, B. (2012) Physical Review D, 86, Article ID: 043520. https://doi.org/10.1103/PhysRevD.86.043520</mixed-citation></ref><ref id="scirp.112694-ref185"><label>185</label><mixed-citation publication-type="other" xlink:type="simple">Chávez, R., et al. (2012) Monthly Notices of the Royal Astronomical Society, 425, L56-L60. https://doi.org/10.1111/j.1745-3933.2012.01299.x</mixed-citation></ref><ref id="scirp.112694-ref186"><label>186</label><mixed-citation publication-type="other" xlink:type="simple">Colless, M., Beutler, F. and Blake, C. (2012) Proceedings of the International Astronomical Union, 8, 319-322. https://doi.org/10.1017/S1743921312021618</mixed-citation></ref><ref id="scirp.112694-ref187"><label>187</label><mixed-citation publication-type="other" xlink:type="simple">Freedman, W.L., et al. (2012) The Astrophysical Journal, 758, Article No. 24. https://doi.org/10.1088/0004-637X/758/1/24</mixed-citation></ref><ref id="scirp.112694-ref188"><label>188</label><mixed-citation publication-type="other" xlink:type="simple">Del Pozzo, W. (2012) Physical Review D, 86, Article ID: 043011. https://doi.org/10.1103/PhysRevD.86.043011</mixed-citation></ref><ref id="scirp.112694-ref189"><label>189</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., Fliri, J. and Valls-Gabaud, D. (2012) The Astrophysical Journal, 745, Article No. 156. https://doi.org/10.1088/0004-637X/745/2/156</mixed-citation></ref><ref id="scirp.112694-ref190"><label>190</label><mixed-citation publication-type="other" xlink:type="simple">Wang, M. (2012) AIP Conference Proceedings, 1441, 503-505. https://doi.org/10.1063/1.3700599</mixed-citation></ref><ref id="scirp.112694-ref191"><label>191</label><mixed-citation publication-type="other" xlink:type="simple">Chen, G. and Ratra, B. (2011) Publications of the Astronomical Society of the Pacific, 123, Article No. 1127. https://doi.org/10.1086/662131</mixed-citation></ref><ref id="scirp.112694-ref192"><label>192</label><mixed-citation publication-type="other" xlink:type="simple">Beutler, F., et al. (2011) Monthly Notices of the Royal Astronomical Society, 416, 3017-3032. https://doi.org/10.1111/j.1365-2966.2011.19250.x</mixed-citation></ref><ref id="scirp.112694-ref193"><label>193</label><mixed-citation publication-type="other" xlink:type="simple">Jarosik, N., et al. (2011) The Astrophysical Journal Supplement Series, 192, Article No. 14. https://doi.org/10.1088/0067-0049/192/2/14</mixed-citation></ref><ref id="scirp.112694-ref194"><label>194</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (2011) The Astrophysical Journal, 730, Article No. 119. https://doi.org/10.1088/0004-637X/730/2/119</mixed-citation></ref><ref id="scirp.112694-ref195"><label>195</label><mixed-citation publication-type="other" xlink:type="simple">Freedman, W.L. and Madore, B.F. (2010) Annual Review of Astronomy and Astrophysics, 48, 673-710. https://doi.org/10.1146/annurev-astro-082708-101829</mixed-citation></ref><ref id="scirp.112694-ref196"><label>196</label><mixed-citation publication-type="other" xlink:type="simple">Paraficz, D. and Hjorth, J. (2010) The Astrophysical Journal, 712, 1378-1384. https://doi.org/10.1088/0004-637X/712/2/1378</mixed-citation></ref><ref id="scirp.112694-ref197"><label>197</label><mixed-citation publication-type="other" xlink:type="simple">Suyu, S.H., et al. (2010) The Astrophysical Journal, 711, 201-221. https://doi.org/10.1088/0004-637X/711/1/201</mixed-citation></ref><ref id="scirp.112694-ref198"><label>198</label><mixed-citation publication-type="other" xlink:type="simple">Hinshaw, G., et al. (2009) The Astrophysical Journal Supplement Series, 180, 225-245. https://doi.org/10.1088/0067-0049/180/2/225</mixed-citation></ref><ref id="scirp.112694-ref199"><label>199</label><mixed-citation publication-type="other" xlink:type="simple">Komatsu, et al. (2009) The Astrophysical Journal Supplement Series, 180, 330-376. https://doi.org/10.1088/0067-0049/180/2/330</mixed-citation></ref><ref id="scirp.112694-ref200"><label>200</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (2009) The Astrophysical Journal, 699, 539-563. https://doi.org/10.1088/0004-637X/699/1/539</mixed-citation></ref><ref id="scirp.112694-ref201"><label>201</label><mixed-citation publication-type="other" xlink:type="simple">Russell, D.G. (2009) Journal of Astrophysics and Astronomy, 30, 93-118. https://doi.org/10.1007/s12036-009-0006-9</mixed-citation></ref><ref id="scirp.112694-ref202"><label>202</label><mixed-citation publication-type="other" xlink:type="simple">Leith, B.M., Ng, S.C.C. and Wiltshir, D.L. (2008) The Astrophysical Journal, 672, L91-L94. https://doi.org/10.1086/527034</mixed-citation></ref><ref id="scirp.112694-ref203"><label>203</label><mixed-citation publication-type="other" xlink:type="simple">Vuissoz, C., et al. (2008) Astronomy &amp; Astrophysics, 488, 481-490. https://doi.org/10.1051/0004-6361:200809866</mixed-citation></ref><ref id="scirp.112694-ref204"><label>204</label><mixed-citation publication-type="other" xlink:type="simple">Oguri, M. (2007) The Astrophysical Journal, 660, 1-15. https://doi.org/10.1086/513093</mixed-citation></ref><ref id="scirp.112694-ref205"><label>205</label><mixed-citation publication-type="other" xlink:type="simple">Spergel, D.N., et al. (2007) The Astrophysical Journal Supplement Series, 170, 377-408. https://doi.org/10.1086/513700</mixed-citation></ref><ref id="scirp.112694-ref206"><label>206</label><mixed-citation publication-type="other" xlink:type="simple">Bonamente, M., Joy, M.K., La Roque, S.J. and Carlstrom, J.E. (2006) The Astrophysical Journal, 647, 25-54. https://doi.org/10.1086/505291</mixed-citation></ref><ref id="scirp.112694-ref207"><label>207</label><mixed-citation publication-type="other" xlink:type="simple">Hütsi, G. (2006) Cosmic Sound: Measuring the Universe with Baryonic Acoustic Oscillations. Dissertation, Ludwig Maximilian University of Munich, München, 1-148, Not Published. (uni-muenchen.de)</mixed-citation></ref><ref id="scirp.112694-ref208"><label>208</label><mixed-citation publication-type="other" xlink:type="simple">Ngeow, C. and Kanbur, S.M. (2006) The Astrophysical Journal, 642, L29-L32. https://doi.org/10.1086/504478</mixed-citation></ref><ref id="scirp.112694-ref209"><label>209</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A., et al. (2006) The Astrophysical Journal, 653, 843-860. https://doi.org/10.1086/508853</mixed-citation></ref><ref id="scirp.112694-ref210"><label>210</label><mixed-citation publication-type="other" xlink:type="simple">Wang, X., Wang, L., Pain, R., Zhou, X. and Li, Z. (2006) The Astrophysical Journal, 645, 488-505. https://doi.org/10.1086/504312</mixed-citation></ref><ref id="scirp.112694-ref211"><label>211</label><mixed-citation publication-type="other" xlink:type="simple">Gibson, B.K. and Brook, C.B. (2005) Symposium—International Astronomical Union, 201, 200-208. https://doi.org/10.1017/S0074180900216264</mixed-citation></ref><ref id="scirp.112694-ref212"><label>212</label><mixed-citation publication-type="book" xlink:type="simple">Hamuy, M. (2005) The Standard Candle Method for Type II Supernovae and the Hubble Constan. In: Marcaide, J.M and Weiler, K.W., Eds., Cosmic Explosions, Vol. 99, Springer, Berlin, Heidelberg, 535-541. https://doi.org/10.1007/3-540-26633-X_71</mixed-citation></ref><ref id="scirp.112694-ref213"><label>213</label><mixed-citation publication-type="other" xlink:type="simple">Magain, P. (2005) Time Delay in Gravitational Lenses: An Alternative Route to the Hubble Constant. Proceedings of ASP Conference Series, Vol. 335, Brussels, 19-22 July 2004, 207-214.</mixed-citation></ref><ref id="scirp.112694-ref214"><label>214</label><mixed-citation publication-type="other" xlink:type="simple">Olivares, G., Atrio-Barandela, F. and Pavón, D. (2005) Physical Review D, 71, Article ID: 063523. https://doi.org/10.1103/PhysRevD.71.063523</mixed-citation></ref><ref id="scirp.112694-ref215"><label>215</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G. (2005) The Astrophysical Journal, 627, 579-607. https://doi.org/10.1086/430497</mixed-citation></ref><ref id="scirp.112694-ref216"><label>216</label><mixed-citation publication-type="other" xlink:type="simple">Schmidt, R.W., Allen, S.W. and Fabian, A.C. (2004) Monthly Notices of the Royal Astronomical Society, 352, 1413-1420. https://doi.org/10.1111/j.1365-2966.2004.08032.x</mixed-citation></ref><ref id="scirp.112694-ref217"><label>217</label><mixed-citation publication-type="other" xlink:type="simple">Stritzinger, M. and Leibundgut, B. (2004) Astronomy &amp; Astrophysics, 431, 423-431. https://doi.org/10.1051/0004-6361:20041630</mixed-citation></ref><ref id="scirp.112694-ref218"><label>218</label><mixed-citation publication-type="other" xlink:type="simple">Udomprasert, P.S., Mason, B.S., Readhead, A.C.S. and Pearson, T.J. (2004) The Astrophysical Journal, 615, 63-81. https://doi.org/10.1086/423946</mixed-citation></ref><ref id="scirp.112694-ref219"><label>219</label><mixed-citation publication-type="other" xlink:type="simple">Boffi, F.R. and Riess, A.G. (2003) The Type Ia Supernova 1998aq and the Hubble Constant. ASP Conference Proceedings, Vol. 303, La Palma, 27-31 May 2002, 101-104.</mixed-citation></ref><ref id="scirp.112694-ref220"><label>220</label><mixed-citation publication-type="other" xlink:type="simple">Dumin, Y.V. (2003) Advances in Space Research, 31, 2461-2466. https://doi.org/10.1016/S0273-1177(03)00533-7</mixed-citation></ref><ref id="scirp.112694-ref221"><label>221</label><mixed-citation publication-type="other" xlink:type="simple">Jimenez, R., Verde, L., Treu, T. and Stern, D. (2003) The Astrophysical Journal, 593, 622-629. https://doi.org/10.1086/376595</mixed-citation></ref><ref id="scirp.112694-ref222"><label>222</label><mixed-citation publication-type="other" xlink:type="simple">Koopmans, L.V.E., Treu, T., Fassnacht, C.D., Blandford, R.D. and Surpi, G. (2003) The Astrophysical Journal, 599, 70-85. https://doi.org/10.1086/379226</mixed-citation></ref><ref id="scirp.112694-ref223"><label>223</label><mixed-citation publication-type="other" xlink:type="simple">Mei, S., Scodeggio, M., Silva, D.R. and Quinn, P.J. (2003) Astronomy and Astrophysics, 399, 441-448. https://doi.org/10.1051/0004-6361:20021800</mixed-citation></ref><ref id="scirp.112694-ref224"><label>224</label><mixed-citation publication-type="other" xlink:type="simple">Saunders, R., et al. (2003) Monthly Notices of the Royal Astronomical Society, 341, 937-940. https://doi.org/10.1046/j.1365-8711.2003.06467.x</mixed-citation></ref><ref id="scirp.112694-ref225"><label>225</label><mixed-citation publication-type="other" xlink:type="simple">Spergel, D.N., et al. (2003) The Astrophysical Journal Supplement Series, 148, 175-174. https://doi.org/10.1086/377226</mixed-citation></ref><ref id="scirp.112694-ref226"><label>226</label><mixed-citation publication-type="other" xlink:type="simple">Fassnacht, C.D., Xanthopoulos, E., Koopmans, L.V.E. and Rusin, D. (2002) The Astrophysical Journal, 581, 823-835. https://doi.org/10.1086/344368</mixed-citation></ref><ref id="scirp.112694-ref227"><label>227</label><mixed-citation publication-type="book" xlink:type="simple">Freedman, W.L. (2002) The Status of the Hubble Constant. In: Metcalfe, N. and Shanks, T., Eds., A New Era in Cosmology. ASP Conference Proceedings, Vol. 283, Astronomical Society of the Pacific, San Francisco, 249-257.</mixed-citation></ref><ref id="scirp.112694-ref228"><label>228</label><mixed-citation publication-type="other" xlink:type="simple">Grainge, K., et al. (2002) Monthly Notices of the Royal Astronomical Society, 333, 318-326. https://doi.org/10.1046/j.1365-8711.2002.05429.x</mixed-citation></ref><ref id="scirp.112694-ref229"><label>229</label><mixed-citation publication-type="other" xlink:type="simple">Kochanek, C.S. (2002) Gravitational Lenses, the Distance Ladder and the Hubble Constant: A New Dark Matter Problem. arXiv:astro-ph/0204043v1.</mixed-citation></ref><ref id="scirp.112694-ref230"><label>230</label><mixed-citation publication-type="other" xlink:type="simple">Tikhonov, N.A. and Galazoutdinova, O.A. (2002) Astrophysics, 45, 253-266.https://doi.org/10.1023/A:1020168130980</mixed-citation></ref><ref id="scirp.112694-ref231"><label>231</label><mixed-citation publication-type="other" xlink:type="simple">Treu, T. and Koopmans, L.V.E. (2002) Monthly Notices of the Royal Astronomical Society, 337, L6-L10. https://doi.org/10.1046/j.1365-8711.2002.06107.x</mixed-citation></ref><ref id="scirp.112694-ref232"><label>232</label><mixed-citation publication-type="other" xlink:type="simple">Freedman, W.L., et al. (2001) The Astrophysical Journal, 553, 47-72. https://doi.org/10.1086/320638</mixed-citation></ref><ref id="scirp.112694-ref233"><label>233</label><mixed-citation publication-type="other" xlink:type="simple">Itoh, N. (2001) The Astronomical Herald, 94, 214-220.</mixed-citation></ref><ref id="scirp.112694-ref234"><label>234</label><mixed-citation publication-type="other" xlink:type="simple">Jensen, J.B., et al. (2001) The Astrophysical Journal, 550, 503-521. https://doi.org/10.1086/319819</mixed-citation></ref><ref id="scirp.112694-ref235"><label>235</label><mixed-citation publication-type="other" xlink:type="simple">Koopmans, L.V.E. and The CLASS Collaboration (2001) Publication of Astronomical Society of Australia, 18, 179-181. https://doi.org/10.1071/AS01024</mixed-citation></ref><ref id="scirp.112694-ref236"><label>236</label><mixed-citation publication-type="other" xlink:type="simple">Liu, M.C. and Graham, J.R. (2001) The Astrophysical Journal, 557, L31-L34. https://doi.org/10.1086/323174</mixed-citation></ref><ref id="scirp.112694-ref237"><label>237</label><mixed-citation publication-type="other" xlink:type="simple">Mason, B.S., Myers, S.T. and Readhead, A.C.S. (2001) The Astrophysical Journal, 555, L11-L15. https://doi.org/10.1086/321737</mixed-citation></ref><ref id="scirp.112694-ref238"><label>238</label><mixed-citation publication-type="other" xlink:type="simple">Mei, S., Quinn, P.J. and Silva, D.R. (2001) Astronomy and Astrophysics, 371, 779-794. https://doi.org/10.1051/0004-6361:20010427</mixed-citation></ref><ref id="scirp.112694-ref239"><label>239</label><mixed-citation publication-type="book" xlink:type="simple">Tonry, J.L. and High-Z Supernova Search Team (2001) Type Ia Supernovae, the Hubble Constant, the Cosmological Constant and the Age of the Universe. In: von Hippel, T., Simpson, C. and Manset, N., Eds., Astrophysical Ages and Times Scales, ASP Conference Series, Vol. 245, San Francisc, Astronomical Society of the Pacific, 593-601.</mixed-citation></ref><ref id="scirp.112694-ref240"><label>240</label><mixed-citation publication-type="other" xlink:type="simple">Willick, J.A. and Batra, P. (2001) The Astrophysical Journal, 548, 564-584. https://doi.org/10.1086/319005</mixed-citation></ref><ref id="scirp.112694-ref241"><label>241</label><mixed-citation publication-type="other" xlink:type="simple">Wang, X.-F., Chen, L. and Li, Z.-W. (2001) Chinese Physics Letters, 18, 154-156. https://doi.org/10.1088/0256-307X/18/1/354</mixed-citation></ref><ref id="scirp.112694-ref242"><label>242</label><mixed-citation publication-type="other" xlink:type="simple">Ferrarese, L., et al. (2000) The Astrophysical Journal, 529, 745-767. https://doi.org/10.1086/308309</mixed-citation></ref><ref id="scirp.112694-ref243"><label>243</label><mixed-citation publication-type="other" xlink:type="simple">Gibson, B.K., et al. (2000) The Astrophysical Journal, 529, 723-744. https://doi.org/10.1086/308306</mixed-citation></ref><ref id="scirp.112694-ref244"><label>244</label><mixed-citation publication-type="other" xlink:type="simple">Mould, J.R., et al. (2000) The Astrophysical Journal, 529, 786-794. https://doi.org/10.1086/308304</mixed-citation></ref><ref id="scirp.112694-ref245"><label>245</label><mixed-citation publication-type="other" xlink:type="simple">Sakai, S. (2000) The Astrophysical Journal, 529, 698-722. https://doi.org/10.1086/308305</mixed-citation></ref><ref id="scirp.112694-ref246"><label>246</label><mixed-citation publication-type="other" xlink:type="simple">Tikhonov, N.A., Galazoutdinova, O.A. and Drozdovskii, I.O. (2000) Astrophysics, 43, 367-380. https://doi.org/10.1023/A:1010902305550</mixed-citation></ref><ref id="scirp.112694-ref247"><label>247</label><mixed-citation publication-type="other" xlink:type="simple">Biggs, A.D., Browne, I.W.A., Helbig, P., Koopmans, L.V.E., Wilkinson, P.N. and Perley, R.A. (1999) Monthly Notices of the Royal Astronomical Society, 304, 349-358. https://doi.org/10.1046/j.1365-8711.1999.02309.x</mixed-citation></ref><ref id="scirp.112694-ref248"><label>248</label><mixed-citation publication-type="other" xlink:type="simple">Chae, K.-H. (1999) The Astrophysical Journal, 524, 582-590. https://doi.org/10.1086/307842</mixed-citation></ref><ref id="scirp.112694-ref249"><label>249</label><mixed-citation publication-type="other" xlink:type="simple">Collier, S., Horne, K., Wanders, I. and Peterson, B.M. (1999) Monthly Notices of the Royal Astronomical Society, 302, L24-L28. https://doi.org/10.1046/j.1365-8711.1999.02250.x</mixed-citation></ref><ref id="scirp.112694-ref250"><label>250</label><mixed-citation publication-type="other" xlink:type="simple">Freedman, W.L. and Feng, L.L. (1999) Proceedings of the National Academy of Sciences of the United States of America, 96, 11063-11064. https://doi.org/10.1073/pnas.96.20.11063</mixed-citation></ref><ref id="scirp.112694-ref251"><label>251</label><mixed-citation publication-type="other" xlink:type="simple">Jha, S., et al. (1999) The Astrophysical Journal Supplement Series, 125, 73-97. https://doi.org/10.1086/313275</mixed-citation></ref><ref id="scirp.112694-ref252"><label>252</label><mixed-citation publication-type="other" xlink:type="simple">Mason, B.S. (1999) An Improved Measurement of the Hubble Constant Using the Sunyaev-Zeldovich Effect. Dissertations, University of Pennsylvania, Philadelphia, UMI Number: AAI9953569. https://repository.upenn.edu/dissertations/AAI9953569</mixed-citation></ref><ref id="scirp.112694-ref253"><label>253</label><mixed-citation publication-type="other" xlink:type="simple">Mazumdar, A. and Narasimba, D. (1999) Bulletin of the Astronomical Society of India, 27, 267.</mixed-citation></ref><ref id="scirp.112694-ref254"><label>254</label><mixed-citation publication-type="other" xlink:type="simple">Tanvir, N.R. (1999) Monthly Notices of the Royal Astronomical Society, 310, 175-188. https://doi.org/10.1046/j.1365-8711.1999.02954.x</mixed-citation></ref><ref id="scirp.112694-ref255"><label>255</label><mixed-citation publication-type="other" xlink:type="simple">Tripp, R. and Branch, D. (1999) The Astrophysical Journal, 525, 209-214. https://doi.org/10.1086/307883</mixed-citation></ref><ref id="scirp.112694-ref256"><label>256</label><mixed-citation publication-type="other" xlink:type="simple">Branch, D. (1998) Annual Review of Astronomy and Astrophysics, 36, 17-55. https://doi.org/10.1146/annurev.astro.36.1.17</mixed-citation></ref><ref id="scirp.112694-ref257"><label>257</label><mixed-citation publication-type="other" xlink:type="simple">Goicoechea, L.J., Mediavilla, E., Oscoz, A., Serra, M. and Buttrago, J. (1998) Astrophysics and Space Science, 261, 341-344. https://doi.org/10.1023/A:1002042026159</mixed-citation></ref><ref id="scirp.112694-ref258"><label>258</label><mixed-citation publication-type="other" xlink:type="simple">Harris, W.E., et al. (1998) Nature, 395, 45-47. https://doi.org/10.1038/25673</mixed-citation></ref><ref id="scirp.112694-ref259"><label>259</label><mixed-citation publication-type="other" xlink:type="simple">Hughes, J.P. and Birkinshaw, M. (1998) The Astrophysical Journal, 501, 1-14. https://doi.org/10.1086/305788</mixed-citation></ref><ref id="scirp.112694-ref260"><label>260</label><mixed-citation publication-type="other" xlink:type="simple">Lauer, T.R., Tonry, J.L., Postman, M., Ajhar, E.A. and Holtzman, J.A. (1998) The Astrophysical Journal, 499, 577-588. https://doi.org/10.1086/305671</mixed-citation></ref><ref id="scirp.112694-ref261"><label>261</label><mixed-citation publication-type="other" xlink:type="simple">Riess, A.G., et al. (1998) The Astronomical Journal, 116, 1009-1038. https://doi.org/10.1086/300499</mixed-citation></ref><ref id="scirp.112694-ref262"><label>262</label><mixed-citation publication-type="book" xlink:type="simple">Tamman, G.A. and Labhardt, L. (1998) A Forty-Year Search for the Hubble Constant. In: Riffert, H., Ruder, H., Nollert, H.P. and Hehl, F.W., Eds., Relativistic Astrophysics, Vieweg+Teubner Verlag, Wiesbaden, 238-261. https://doi.org/10.1007/978-3-663-11294-5_15</mixed-citation></ref><ref id="scirp.112694-ref263"><label>263</label><mixed-citation publication-type="other" xlink:type="simple">Tripp, R. (1998) Astronomy and Astrophysics, 331, 815-820.</mixed-citation></ref><ref id="scirp.112694-ref264"><label>264</label><mixed-citation publication-type="other" xlink:type="simple">Giovanelli, R. (1997) The Extragalactic Distance Scale. Proceedings of the ST ScI May Symposium, Baltimore, 7-10 May 1996, 113.</mixed-citation></ref><ref id="scirp.112694-ref265"><label>265</label><mixed-citation publication-type="other" xlink:type="simple">Gregg, M.D. (1997) New Astronomy, 1, 363-371. https://doi.org/10.1016/S1384-1076(97)00005-5</mixed-citation></ref><ref id="scirp.112694-ref266"><label>266</label><mixed-citation publication-type="other" xlink:type="simple">Hjorth, J. and Tanvir, N.R. (1997) The Astrophysical Journal, 482, 68-74. https://doi.org/10.1086/304124</mixed-citation></ref><ref id="scirp.112694-ref267"><label>267</label><mixed-citation publication-type="other" xlink:type="simple">Holzapfel, W.L., et al. (1997) The Astrophysical Journal, 480, 449-465. https://doi.org/10.1086/303979</mixed-citation></ref><ref id="scirp.112694-ref268"><label>268</label><mixed-citation publication-type="other" xlink:type="simple">Hoyle, F., Burhidge, G. and Narlikar, J.V. (1997) Monthly Notices of the Royal Astronomical Society, 286, 173-182. https://doi.org/10.1093/mnras/286.1.173</mixed-citation></ref><ref id="scirp.112694-ref269"><label>269</label><mixed-citation publication-type="other" xlink:type="simple">Schechter, P.L. (1997) The Astrophysical Journal, 475, L85-L88.https://doi.org/10.1086/310478</mixed-citation></ref><ref id="scirp.112694-ref270"><label>270</label><mixed-citation publication-type="other" xlink:type="simple">Sciama, D.W. (1997) Monthly Notices of the Royal Astronomical Society, 289, 945-947. https://doi.org/10.1093/mnras/289.4.945</mixed-citation></ref><ref id="scirp.112694-ref271"><label>271</label><mixed-citation publication-type="other" xlink:type="simple">Tonry, J.L., Blakeslee, J.P., Ajhar, E.A. and Dressler, A. (1997) The Astrophysical Journal, 475, 399-413. https://doi.org/10.1086/303576</mixed-citation></ref><ref id="scirp.112694-ref272"><label>272</label><mixed-citation publication-type="other" xlink:type="simple">Amendola, L. (1996) Astronomy and Astrophysics, 312, 353-356.</mixed-citation></ref><ref id="scirp.112694-ref273"><label>273</label><mixed-citation publication-type="other" xlink:type="simple">Biesiada, M. (1996) Monthly Notices of the Royal Astronomical Society, 283, 997-982. https://doi.org/10.1093/mnras/283.3.977</mixed-citation></ref><ref id="scirp.112694-ref274"><label>274</label><mixed-citation publication-type="other" xlink:type="simple">Forbes, D.A., Brodie, J.P. and Huchra, J. (1996) Astronomical Journal, 112, 2448-2460. https://doi.org/10.1086/118194</mixed-citation></ref><ref id="scirp.112694-ref275"><label>275</label><mixed-citation publication-type="other" xlink:type="simple">Kobyashi, S., Sasaki, S. and Suto, Y. (1996) Publications of the Astronomical Society of Japan, 48, L107-L111. https://doi.org/10.1093/pasj/48.6.L107</mixed-citation></ref><ref id="scirp.112694-ref276"><label>276</label><mixed-citation publication-type="other" xlink:type="simple">Mallik, D.C.V. (1996) Current Science, 71, 547-552.https://www.jstor.org/stable/24098091</mixed-citation></ref><ref id="scirp.112694-ref277"><label>277</label><mixed-citation publication-type="other" xlink:type="simple">Schaefer, B.E. (1996) The Astrophysical Journal, 460, L19-L23. https://doi.org/10.1086/309963</mixed-citation></ref><ref id="scirp.112694-ref278"><label>278</label><mixed-citation publication-type="other" xlink:type="simple">Grogin, N.A. and Narayan, R. (1995) The Astrophysical Journal, 473, 570-571. https://doi.org/10.1086/178171</mixed-citation></ref><ref id="scirp.112694-ref279"><label>279</label><mixed-citation publication-type="other" xlink:type="simple">Herbig, T., Lawrence, C.R., Readhead, A.C.S. and Gulkis, S. (1995) The Astrophysical Journal, 449, L5-L8. https://doi.org/10.1086/309616</mixed-citation></ref><ref id="scirp.112694-ref280"><label>280</label><mixed-citation publication-type="other" xlink:type="simple">Holzapfel, W.L., et al. (1995) Bulletin of the American Astronomical Society, 27, 1413.</mixed-citation></ref><ref id="scirp.112694-ref281"><label>281</label><mixed-citation publication-type="other" xlink:type="simple">Jones, M. (1995) Astrophysical Letters and Communications, 32, 347-353.</mixed-citation></ref><ref id="scirp.112694-ref282"><label>282</label><mixed-citation publication-type="other" xlink:type="simple">Kennicutt Jr., R.C., Freedman, W.L. and Mould, J.R. (1995) The Astrophysical Journal, 110, 1476-1491. https://doi.org/10.1086/117621</mixed-citation></ref><ref id="scirp.112694-ref283"><label>283</label><mixed-citation publication-type="other" xlink:type="simple">Mould, J., et al. (1995) The Astrophysical Journal, 449, 413-421.</mixed-citation></ref><ref id="scirp.112694-ref284"><label>284</label><mixed-citation publication-type="other" xlink:type="simple">Nakamura, T.T. and Suto, Y. (1995) Astrophysical Journal Letters, 447, L65-L68. https://doi.org/10.1086/309580</mixed-citation></ref><ref id="scirp.112694-ref285"><label>285</label><mixed-citation publication-type="other" xlink:type="simple">Raphaeli, Y. (1995) Annual Review of Astronomy and Astrophysics, 33, 541-579. https://doi.org/10.1146/annurev.aa.33.090195.002545</mixed-citation></ref><ref id="scirp.112694-ref286"><label>286</label><mixed-citation publication-type="other" xlink:type="simple">Scheafer, B.E. (1995) The Astrophysical Journal, 447, L13-L16.</mixed-citation></ref><ref id="scirp.112694-ref287"><label>287</label><mixed-citation publication-type="other" xlink:type="simple">Tanvir, N.R., Shanks, T., Ferguson, H.C. and Robinson, D.R.T. (1995) Nature, 377, 27-31. https://doi.org/10.1038/377027a0</mixed-citation></ref><ref id="scirp.112694-ref288"><label>288</label><mixed-citation publication-type="other" xlink:type="simple">Whitmore, B.C. and Schweizer, F. (1995) The Astronomical Journal, 210, 960-980 and 1411-1416 (For Graphics).</mixed-citation></ref><ref id="scirp.112694-ref289"><label>289</label><mixed-citation publication-type="other" xlink:type="simple">Birkinshaw, M. and Hughes, J.P. (1994) The Astrophysical Journal, 420, 33-43. https://doi.org/10.1086/173540</mixed-citation></ref><ref id="scirp.112694-ref290"><label>290</label><mixed-citation publication-type="other" xlink:type="simple">Freedman, W., et al. (1994) Nature, 371, 757-762. https://doi.org/10.1038/371757a0</mixed-citation></ref><ref id="scirp.112694-ref291"><label>291</label><mixed-citation publication-type="other" xlink:type="simple">Lu, N.Y., Salpeter, E.E. and Hoffman, G.L. (1994) The Astrophysical Journal, 426, 473-485. https://doi.org/10.1086/174083</mixed-citation></ref><ref id="scirp.112694-ref292"><label>292</label><mixed-citation publication-type="other" xlink:type="simple">Schmidt, B.P., et al. (1994) Astrophysical Journal, 432, 42-48.</mixed-citation></ref><ref id="scirp.112694-ref293"><label>293</label><mixed-citation publication-type="other" xlink:type="simple">Tully, R.B. (1993) Proceedings of the National Academy of Sciences of the United States of America, 90, 4806-4810. https://doi.org/10.1073/pnas.90.11.4806</mixed-citation></ref><ref id="scirp.112694-ref294"><label>294</label><mixed-citation publication-type="other" xlink:type="simple">Duemmler, R. (1992) Astronomy and Astrophysics, 264, 1-10.</mixed-citation></ref><ref id="scirp.112694-ref295"><label>295</label><mixed-citation publication-type="other" xlink:type="simple">Lauer, T.D. and Postman, M. (1992) The Astrophysical Journal, 400, L47. https://doi.org/10.1086/186646</mixed-citation></ref><ref id="scirp.112694-ref296"><label>296</label><mixed-citation publication-type="other" xlink:type="simple">Leibundgut, B. and Pinto, P. (1992) The Astrophysical Journal, 401, 49-59. https://doi.org/10.1086/172037</mixed-citation></ref><ref id="scirp.112694-ref297"><label>297</label><mixed-citation publication-type="other" xlink:type="simple">Birkinshaw, M., Hughes, J.P. and Arnaud, K.A. (1991) The Astrophysical Journal, 379, 466-481. https://doi.org/10.1086/170522</mixed-citation></ref><ref id="scirp.112694-ref298"><label>298</label><mixed-citation publication-type="other" xlink:type="simple">Tonry, J.L. (1991) Astrophysical Journal Letters, 373, L1. https://doi.org/10.1086/186037</mixed-citation></ref><ref id="scirp.112694-ref299"><label>299</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A. and Tammann, G.A. (1990) The Astrophysical Journal, 365, 1-12. https://doi.org/10.1086/169453</mixed-citation></ref><ref id="scirp.112694-ref300"><label>300</label><mixed-citation publication-type="other" xlink:type="simple">Visvanathan, N. (1990) Australian Journal of Physics, 43, 189-210. https://doi.org/10.1071/PH900189</mixed-citation></ref><ref id="scirp.112694-ref301"><label>301</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A. and Tammann, G. (1988) The Astrophysical Journal, 328, 1-3. https://doi.org/10.1086/166263</mixed-citation></ref><ref id="scirp.112694-ref302"><label>302</label><mixed-citation publication-type="other" xlink:type="simple">Dressler, A. (1987) The Astrophysical Journal, 317, 1-10. https://doi.org/10.1086/165251</mixed-citation></ref><ref id="scirp.112694-ref303"><label>303</label><mixed-citation publication-type="other" xlink:type="simple">Tamman, G.A. and Sandage, A. (1985) The Astrophysical Journal, 294, 81-95. https://doi.org/10.1086/163277</mixed-citation></ref><ref id="scirp.112694-ref304"><label>304</label><mixed-citation publication-type="other" xlink:type="simple">Visvanathan, N. (1983) The Astrophysical Journal, 275, 430-444. https://doi.org/10.1086/161544</mixed-citation></ref><ref id="scirp.112694-ref305"><label>305</label><mixed-citation publication-type="other" xlink:type="simple">Hanes, D.A. (1979) Monthly Notices of the Royal Astronomical Society, 188, 901-909. https://doi.org/10.1093/mnras/188.4.901</mixed-citation></ref><ref id="scirp.112694-ref306"><label>306</label><mixed-citation publication-type="other" xlink:type="simple">Bottinelli, L. and Gouguenheim, L. (1976) Astronomy and Astrophysics, 51, 275-306.</mixed-citation></ref><ref id="scirp.112694-ref307"><label>307</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A. and Tammann, G.A. (1976) The Astrophysical Journal, 210, 7-24. https://doi.org/10.1086/154798</mixed-citation></ref><ref id="scirp.112694-ref308"><label>308</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A. and Tammann, G.A. (1975) The Astrophysical Journal, 197, 265-280. https://doi.org/10.1086/153510</mixed-citation></ref><ref id="scirp.112694-ref309"><label>309</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A. and Tammann, G.A. (1974) The Astrophysical Journal, 194, 559-568. https://doi.org/10.1086/153275</mixed-citation></ref><ref id="scirp.112694-ref310"><label>310</label><mixed-citation publication-type="other" xlink:type="simple">Sandage, A. and Tammann, G.A. (1974) The Astrophysical Journal, 194, 223-243. https://doi.org/10.1086/153238</mixed-citation></ref></ref-list></back></article>