<?xml version="1.0" encoding="ISO-8859-1"?><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance">
<front>
<journal-meta>
<journal-id>0035-001X</journal-id>
<journal-title><![CDATA[Revista mexicana de física]]></journal-title>
<abbrev-journal-title><![CDATA[Rev. mex. fis.]]></abbrev-journal-title>
<issn>0035-001X</issn>
<publisher>
<publisher-name><![CDATA[Sociedad Mexicana de Física]]></publisher-name>
</publisher>
</journal-meta>
<article-meta>
<article-id>S0035-001X2022000400003</article-id>
<article-id pub-id-type="doi">10.31349/revmexfis.68.040702</article-id>
<title-group>
<article-title xml:lang="en"><![CDATA[A dynamical dark energy solution to hubble tension in the light of the multimessenger era]]></article-title>
</title-group>
<contrib-group>
<contrib contrib-type="author">
<name>
<surname><![CDATA[Escamilla-Rivera]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
<xref ref-type="aff" rid="Aff"/>
</contrib>
</contrib-group>
<aff id="Af1">
<institution><![CDATA[,Universidad Nacional Autónoma de México Instituto de Ciencias Nucleares ]]></institution>
<addr-line><![CDATA[Cuidad de México ]]></addr-line>
<country>Mexico</country>
</aff>
<pub-date pub-type="pub">
<day>00</day>
<month>08</month>
<year>2022</year>
</pub-date>
<pub-date pub-type="epub">
<day>00</day>
<month>08</month>
<year>2022</year>
</pub-date>
<volume>68</volume>
<numero>4</numero>
<copyright-statement/>
<copyright-year/>
<self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_arttext&amp;pid=S0035-001X2022000400003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_abstract&amp;pid=S0035-001X2022000400003&amp;lng=en&amp;nrm=iso"></self-uri><self-uri xlink:href="http://www.scielo.org.mx/scielo.php?script=sci_pdf&amp;pid=S0035-001X2022000400003&amp;lng=en&amp;nrm=iso"></self-uri><abstract abstract-type="short" xml:lang="en"><p><![CDATA[Abstract We show that the gravitational waves measurements have raised the opportunity to measure H 0 with dark sirens to within 2&#963;, the accuracy required to resolve the Hubble-Lemaître tension. There are two principal reasons for our results: (1) upgrades to GW LIGO-Virgo transient catalogues GWTC-1 and GWTC-2 enhance their sensitive with only 10% of contamination fraction, and (2) new dark sirens should help to constrain our dynamical EoS. In conjunction, sensitivity upgrades and a new dark energy model will facilitate an accurate inference of the Hubble-Lemaître constant H 0 to better with an ±0.077 error in comparison to the LIGO dark siren with +14.0/-7.0, which would further solidify the role of dark sirens in late dark energy for precision cosmology in the future.]]></p></abstract>
<kwd-group>
<kwd lng="en"><![CDATA[Gravitational waves]]></kwd>
<kwd lng="en"><![CDATA[GWTC-1]]></kwd>
<kwd lng="en"><![CDATA[GWTC-2]]></kwd>
</kwd-group>
</article-meta>
</front><back>
<ref-list>
<ref id="B1">
<label>1</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ade]]></surname>
<given-names><![CDATA[P. A. R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Planck 2013 results. XVI. Cosmological parameters]]></article-title>
<source><![CDATA[Astron. Astrophys.]]></source>
<year>2014</year>
<volume>571</volume>
<page-range>A16</page-range></nlm-citation>
</ref>
<ref id="B2">
<label>2</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Riess]]></surname>
<given-names><![CDATA[A. G.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A space telescopeand wide field camera 3]]></article-title>
<source><![CDATA[The Astrophysical Journal]]></source>
<year>2011</year>
<volume>730</volume>
<page-range>119</page-range></nlm-citation>
</ref>
<ref id="B3">
<label>3</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Aghanim]]></surname>
<given-names><![CDATA[N.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Planck 2018 results. VI. Cosmological parameters]]></article-title>
<source><![CDATA[Astron. Astrophys.]]></source>
<year>2020</year>
<volume>641</volume>
<page-range>A6</page-range></nlm-citation>
</ref>
<ref id="B4">
<label>4</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Riess]]></surname>
<given-names><![CDATA[A. G.]]></given-names>
</name>
<name>
<surname><![CDATA[Casertano]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Yuan]]></surname>
<given-names><![CDATA[W.]]></given-names>
</name>
<name>
<surname><![CDATA[Macri]]></surname>
<given-names><![CDATA[L. M.]]></given-names>
</name>
<name>
<surname><![CDATA[Scolnic]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond (]]></article-title>
<source><![CDATA[Astrophys. J.]]></source>
<year>2019</year>
<volume>876</volume>
<page-range>85</page-range></nlm-citation>
</ref>
<ref id="B5">
<label>5</label><nlm-citation citation-type="book">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Verde]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<name>
<surname><![CDATA[Treu]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
<name>
<surname><![CDATA[Riess]]></surname>
<given-names><![CDATA[A. G.]]></given-names>
</name>
</person-group>
<source><![CDATA[Tensions between the Early and the Late Universe]]></source>
<year>2019</year>
<publisher-name><![CDATA[In Nature Astronomy]]></publisher-name>
</nlm-citation>
</ref>
<ref id="B6">
<label>6</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Chen]]></surname>
<given-names><![CDATA[G. C. F.]]></given-names>
</name>
</person-group>
<source><![CDATA[A SHARP view of H0LiCOW: H0 from three time-delay gravitational lens systems with adaptive optics imaging]]></source>
<year>2019</year>
</nlm-citation>
</ref>
<ref id="B7">
<label>7</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Wong]]></surname>
<given-names><![CDATA[Kenneth C.]]></given-names>
</name>
</person-group>
<source><![CDATA[H0LiCOW XIII. A 2.4% measurement of H0 from lensed quasars: 5:3( tension between early and late-Universe probes]]></source>
<year>2019</year>
</nlm-citation>
</ref>
<ref id="B8">
<label>8</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Suyu]]></surname>
<given-names><![CDATA[S. H.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[H0LiCOW I. H0 Lenses in COSMOGRAIL&#8217;s Wellspring: program overview]]></article-title>
<source><![CDATA[Mon. Not. Roy. Astron. Soc.]]></source>
<year>2017</year>
<volume>468</volume>
<page-range>2590</page-range></nlm-citation>
</ref>
<ref id="B9">
<label>9</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[T. M. C.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[The Dark Energy Survey Data Release 1]]></article-title>
<source><![CDATA[Astrophys. J. Suppl.]]></source>
<year>2018</year>
<volume>239</volume>
<page-range>18</page-range></nlm-citation>
</ref>
<ref id="B10">
<label>10</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Macaulay]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[First Cosmological Results using Type Ia Supernovae from the Dark Energy Survey: Measurement of the Hubble Constant]]></article-title>
<source><![CDATA[Mon. Not. Roy. Astron. Soc.]]></source>
<year>2019</year>
<volume>486</volume>
<page-range>2184</page-range></nlm-citation>
</ref>
<ref id="B11">
<label>11</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Reid]]></surname>
<given-names><![CDATA[M. J.]]></given-names>
</name>
<name>
<surname><![CDATA[Pesce]]></surname>
<given-names><![CDATA[D. W.]]></given-names>
</name>
<name>
<surname><![CDATA[Riess]]></surname>
<given-names><![CDATA[A. G.]]></given-names>
</name>
</person-group>
<source><![CDATA[An Improved Distance to NGC 4258 and its Implications for the Hubble Constant]]></source>
<year>2019</year>
</nlm-citation>
</ref>
<ref id="B12">
<label>12</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Borhanian]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Dhani]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Gupta]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Arun]]></surname>
<given-names><![CDATA[K. G.]]></given-names>
</name>
<name>
<surname><![CDATA[Sathyaprakash]]></surname>
<given-names><![CDATA[B. S.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Dark Sirens to Resolve the 10 Hubble-Lemaître Tension]]></article-title>
<source><![CDATA[Astrophys. J. Lett.]]></source>
<year>2020</year>
<volume>905</volume>
<page-range>L28</page-range></nlm-citation>
</ref>
<ref id="B13">
<label>13</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Haslbauer]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Banik]]></surname>
<given-names><![CDATA[I.]]></given-names>
</name>
<name>
<surname><![CDATA[Kroupa]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[The KBC void and Hubble tension contradict &#120549;CDM on a Gpc scale Milgromian dynamics as a possible solution]]></article-title>
<source><![CDATA[Mon. Not. Roy. Astron. Soc.]]></source>
<year>2020</year>
<volume>499</volume>
<page-range>2845</page-range></nlm-citation>
</ref>
<ref id="B14">
<label>14</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Kenworthy]]></surname>
<given-names><![CDATA[W. D&#8217;Arcy]]></given-names>
</name>
<name>
<surname><![CDATA[Scolnic]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Riess]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[The Local Perspective on the Hubble Tension: Local Structure Does Not Impact Measurement of the Hubble Constant]]></article-title>
<source><![CDATA[Astrophys. J.]]></source>
<year>2019</year>
<volume>875</volume>
<page-range>145</page-range></nlm-citation>
</ref>
<ref id="B15">
<label>15</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Shanks]]></surname>
<given-names><![CDATA[T.]]></given-names>
</name>
<name>
<surname><![CDATA[Hogarth]]></surname>
<given-names><![CDATA[L.]]></given-names>
</name>
<name>
<surname><![CDATA[Metcalfe]]></surname>
<given-names><![CDATA[N.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Gaia Cepheid parallaxes and &#8217;Local Hole&#8217; relieve H0 tension]]></article-title>
<source><![CDATA[Mon. Not. Roy. Astron. Soc.]]></source>
<year>2019</year>
<volume>484</volume>
<page-range>L64</page-range></nlm-citation>
</ref>
<ref id="B16">
<label>16</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Valentino]]></surname>
<given-names><![CDATA[E. Di]]></given-names>
</name>
</person-group>
<source><![CDATA[Cosmology Intertwined II: The Hubble Constant Tension]]></source>
<year>2020</year>
<volume>8</volume>
</nlm-citation>
</ref>
<ref id="B17">
<label>17</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Mészáros]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
<name>
<surname><![CDATA[Fox]]></surname>
<given-names><![CDATA[D. B.]]></given-names>
</name>
<name>
<surname><![CDATA[Hanna]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
<name>
<surname><![CDATA[Murase]]></surname>
<given-names><![CDATA[K.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Multi-Messenger Astrophysics]]></article-title>
<source><![CDATA[Nature Rev. Phys.]]></source>
<year>2019</year>
<volume>1</volume>
<page-range>585</page-range></nlm-citation>
</ref>
<ref id="B18">
<label>18</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Ezquiaga]]></surname>
<given-names><![CDATA[J. M.]]></given-names>
</name>
<name>
<surname><![CDATA[Zumalacárregui]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Dark Energy in light of Multi-Messenger Gravitational-Wave astronomy]]></article-title>
<source><![CDATA[Front. Astron. Space Sci.]]></source>
<year>2018</year>
<volume>5</volume>
<page-range>44</page-range></nlm-citation>
</ref>
<ref id="B19">
<label>19</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Corman]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Escamilla-Rivera]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
<name>
<surname><![CDATA[Hendry]]></surname>
<given-names><![CDATA[M. A.]]></given-names>
</name>
</person-group>
<source><![CDATA[Constraining extra dimensions on cosmological scales with LISA future gravitational wave siren data]]></source>
<year>2020</year>
<volume>4</volume>
</nlm-citation>
</ref>
<ref id="B20">
<label>20</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[B. P.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A gravitational-wave standard siren measurement of the Hubble constant]]></article-title>
<source><![CDATA[Nature]]></source>
<year>2017</year>
<volume>551</volume>
<page-range>85</page-range></nlm-citation>
</ref>
<ref id="B21">
<label>21</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[B. P.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral]]></article-title>
<source><![CDATA[Phys. Rev. Lett.]]></source>
<year>2017</year>
<volume>119</volume>
<page-range>161101</page-range></nlm-citation>
</ref>
<ref id="B22">
<label>22</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[B. P.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs]]></article-title>
<source><![CDATA[Phys. Rev. X]]></source>
<year>2019</year>
<volume>9</volume>
<page-range>031040</page-range></nlm-citation>
</ref>
<ref id="B23">
<label>23</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Hotokezaka]]></surname>
<given-names><![CDATA[Kenta]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A Hubble constant measurement from superluminal motion of the jet in GW170817]]></article-title>
<source><![CDATA[Nature Astron.]]></source>
<year>2019</year>
</nlm-citation>
</ref>
<ref id="B24">
<label>24</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Niedermann]]></surname>
<given-names><![CDATA[F.]]></given-names>
</name>
<name>
<surname><![CDATA[Sloth]]></surname>
<given-names><![CDATA[M. S.]]></given-names>
</name>
</person-group>
<source><![CDATA[New Early Dark Energy]]></source>
<year>2019</year>
<volume>10</volume>
</nlm-citation>
</ref>
<ref id="B25">
<label>25</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Chevallier]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
<name>
<surname><![CDATA[Polarski]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Accelerating universes with scaling dark matter]]></article-title>
<source><![CDATA[Int. J. Mod. Phys. D]]></source>
<year>2001</year>
<volume>10</volume>
<page-range>213</page-range></nlm-citation>
</ref>
<ref id="B26">
<label>26</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Linder]]></surname>
<given-names><![CDATA[Eric V.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[The Dynamics of Quintessence, The Quintessence of Dynamics]]></article-title>
<source><![CDATA[Gen. Rel. Grav.]]></source>
<year>2008</year>
<volume>40</volume>
<page-range>329</page-range></nlm-citation>
</ref>
<ref id="B27">
<label>27</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Barboza J.r.]]></surname>
<given-names><![CDATA[E. M.]]></given-names>
</name>
<name>
<surname><![CDATA[Alcaniz]]></surname>
<given-names><![CDATA[J.S.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A parametric model for dark energy]]></article-title>
<source><![CDATA[Physics Letters B]]></source>
<year>2008</year>
<volume>666</volume>
<page-range>415</page-range></nlm-citation>
</ref>
<ref id="B28">
<label>28</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Yang]]></surname>
<given-names><![CDATA[W.]]></given-names>
</name>
<name>
<surname><![CDATA[Pan]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Valentino]]></surname>
<given-names><![CDATA[E. Di]]></given-names>
</name>
<name>
<surname><![CDATA[Saridakis]]></surname>
<given-names><![CDATA[E. N.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Observational constraints on dynamical dark energy with pivoting redshift]]></article-title>
<source><![CDATA[Universe]]></source>
<year>2019</year>
<volume>5</volume>
<page-range>219</page-range></nlm-citation>
</ref>
<ref id="B29">
<label>29</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Schutz]]></surname>
<given-names><![CDATA[B. F.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Determining the Hubble Constant from Gravitational Wave Observations]]></article-title>
<source><![CDATA[Nature]]></source>
<year>1986</year>
<volume>323</volume>
<page-range>310</page-range></nlm-citation>
</ref>
<ref id="B30">
<label>30</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Holz]]></surname>
<given-names><![CDATA[D. E.]]></given-names>
</name>
<name>
<surname><![CDATA[Hughes]]></surname>
<given-names><![CDATA[S. A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Using gravitational-wave standard sirens]]></article-title>
<source><![CDATA[Astrophys. J.]]></source>
<year>2005</year>
<volume>629</volume>
<page-range>15</page-range></nlm-citation>
</ref>
<ref id="B31">
<label>31</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Gray]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Cosmological inference using gravitational wave standard sirens: A mock data analysis]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2020</year>
<volume>101</volume>
<page-range>122001</page-range></nlm-citation>
</ref>
<ref id="B32">
<label>32</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[B. P.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo]]></article-title>
<source><![CDATA[Astrophys. J.]]></source>
<year>2021</year>
<volume>909</volume>
<page-range>218</page-range></nlm-citation>
</ref>
<ref id="B33">
<label>33</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Pozzo]]></surname>
<given-names><![CDATA[W. Del]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Inference of the cosmological parameters from gravitational waves: application to second generation interferometers]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2012</year>
<volume>86</volume>
<page-range>043011</page-range></nlm-citation>
</ref>
<ref id="B34">
<label>34</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
</person-group>
<source><![CDATA[Search of the Early O3 LIGO Data for Continuous Gravitational Waves from the Cassiopeia A and Vela Jr. Supernova Remnants]]></source>
<year>2021</year>
<volume>11</volume>
</nlm-citation>
</ref>
<ref id="B35">
<label>35</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Gupta]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Fox]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Sathyaprakash]]></surname>
<given-names><![CDATA[B. S.]]></given-names>
</name>
<name>
<surname><![CDATA[Schutz]]></surname>
<given-names><![CDATA[B. F.]]></given-names>
</name>
</person-group>
<source><![CDATA[Calibrating the cosmic distance ladder using gravitational-wave observations]]></source>
<year>2019</year>
<volume>10</volume>
</nlm-citation>
</ref>
<ref id="B36">
<label>36</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Nishizawa]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Measurement of Hubble constant with stellar-mass binary black holes]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2017</year>
<volume>96</volume>
<page-range>101303</page-range></nlm-citation>
</ref>
<ref id="B37">
<label>37</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Nair]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
<name>
<surname><![CDATA[Bose]]></surname>
<given-names><![CDATA[S.]]></given-names>
</name>
<name>
<surname><![CDATA[Saini]]></surname>
<given-names><![CDATA[T. Deep]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Measuring the Hubble constant: Gravitational wave observations meet galaxy clustering]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2018</year>
<volume>98</volume>
<page-range>023502</page-range></nlm-citation>
</ref>
<ref id="B38">
<label>38</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
</person-group>
<source><![CDATA[GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run]]></source>
<year>2020</year>
<volume>10</volume>
</nlm-citation>
</ref>
<ref id="B39">
<label>39</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[GW190412: Observation of a Binary-Black-Hole Coalescence with Asymmetric Masses]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2020</year>
<volume>102</volume>
<page-range>043015</page-range></nlm-citation>
</ref>
<ref id="B40">
<label>40</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[R.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[GW190814: Gravitational Waves from the Co-alescence of a 23 Solar Mass Black Hole with a 2.6 Solar Mass Compact Object]]></article-title>
<source><![CDATA[Astrophys. J. Lett.]]></source>
<year>2020</year>
<volume>896</volume>
<page-range>L44</page-range></nlm-citation>
</ref>
<ref id="B41">
<label>41</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Scolnic]]></surname>
<given-names><![CDATA[D. M.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample]]></article-title>
<source><![CDATA[Astrophys. J.]]></source>
<year>2018</year>
<volume>859</volume>
<page-range>101</page-range></nlm-citation>
</ref>
<ref id="B42">
<label>42</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Moresco]]></surname>
<given-names><![CDATA[M.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[A 6% measurement of the Hubble parameter at z (0.45 direct evidence of the epoch of cosmic re-acceleration]]></article-title>
<source><![CDATA[JCAP]]></source>
<year>2016</year>
<volume>05</volume>
<page-range>014</page-range></nlm-citation>
</ref>
<ref id="B43">
<label>43</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Abbott]]></surname>
<given-names><![CDATA[P.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Gwtc-1: a gravitational-wave transient catalog of compact binary mergers observed by ligo and virgo during the first and second observing runs]]></article-title>
<source><![CDATA[Phys. Rev. X]]></source>
<year>2019</year>
<volume>9</volume>
<page-range>031040</page-range></nlm-citation>
</ref>
<ref id="B44">
<label>44</label><nlm-citation citation-type="">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Mitra]]></surname>
<given-names><![CDATA[A.]]></given-names>
</name>
<name>
<surname><![CDATA[Mifsud]]></surname>
<given-names><![CDATA[J.]]></given-names>
</name>
<name>
<surname><![CDATA[Mota]]></surname>
<given-names><![CDATA[D. F.]]></given-names>
</name>
<name>
<surname><![CDATA[Parkinson]]></surname>
</name>
</person-group>
<source><![CDATA[Cosmology with the Einstein Telescope: No Slip Gravity Model and Redshift Specifications]]></source>
<year>2020</year>
<volume>9</volume>
</nlm-citation>
</ref>
<ref id="B45">
<label>45</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Escamilla-Rivera]]></surname>
<given-names><![CDATA[C.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Status on bidimensional dark energy parameterizations using SNe Ia JLA and BAO datasets]]></article-title>
<source><![CDATA[Galaxies]]></source>
<year>2016</year>
<volume>4</volume>
<page-range>8</page-range></nlm-citation>
</ref>
<ref id="B46">
<label>46</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Huterer]]></surname>
<given-names><![CDATA[D.]]></given-names>
</name>
<name>
<surname><![CDATA[Turner]]></surname>
<given-names><![CDATA[M. S.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Probing dark energy: Methods and strategies]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2001</year>
<volume>64</volume>
<page-range>123527</page-range></nlm-citation>
</ref>
<ref id="B47">
<label>47</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Wang]]></surname>
<given-names><![CDATA[Y.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Figure of merit for dark energy constraints from current observational data]]></article-title>
<source><![CDATA[Phys. Rev. D]]></source>
<year>2008</year>
<volume>77</volume>
<page-range>123525</page-range></nlm-citation>
</ref>
<ref id="B48">
<label>48</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Wetterich]]></surname>
<given-names><![CDATA[Christof]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Phenomenological parameterization of quintessence]]></article-title>
<source><![CDATA[Physics Letters B]]></source>
<year>2004</year>
<volume>594</volume>
<page-range>17</page-range></nlm-citation>
</ref>
<ref id="B49">
<label>49</label><nlm-citation citation-type="journal">
<person-group person-group-type="author">
<name>
<surname><![CDATA[Belgacem]]></surname>
<given-names><![CDATA[E.]]></given-names>
</name>
</person-group>
<article-title xml:lang=""><![CDATA[Testing modified gravity at cosmological distances with lisa standard sirens]]></article-title>
<source><![CDATA[Journal of Cosmology and Astroparticle Physics]]></source>
<year>2019</year>
<volume>2019</volume>
<page-range>024</page-range></nlm-citation>
</ref>
</ref-list>
</back>
</article>
