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<ri:Resource created="2024-10-21T14:07:52Z" status="active" updated="2025-06-13T15:25:00Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>The Pantheon+ analysis: cosmological constraints</title><shortName>J/ApJ/938/110</shortName><identifier>ivo://CDS.VizieR/J/ApJ/938/110</identifier><altIdentifier>doi:10.26093/cds/vizier.19380110</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Brout D.</name></creator><creator><name>Scolnic D.</name></creator><creator><name>Popovic B.</name></creator><creator><name>Riess A.G.</name></creator><creator><name>Carr A.</name></creator><creator><name>Zuntz J.,Kessler R.</name></creator><creator><name>Davis T.M.</name></creator><creator><name>Hinton S.</name></creator><creator><name>Jones D.</name></creator><creator><name>Kenworthy W.D.,Peterson E.R.</name></creator><creator><name>Said K.</name></creator><creator><name>Taylor G.</name></creator><creator><name>Ali N.</name></creator><creator><name>Armstrong P.</name></creator><creator><name>Charvu P.,Dwomoh A.</name></creator><creator><name>Meldorf C.</name></creator><creator><name>Palmese A.</name></creator><creator><name>Qu H.</name></creator><creator><name>Rose B.M.</name></creator><creator><name>Sanchez B.,Stubbs C.W.</name></creator><creator><name>Vincenzi M.</name></creator><creator><name>Wood C.M.</name></creator><creator><name>Brown P.J.</name></creator><creator><name>Chen R.</name></creator><creator><name>Chambers K.,Coulter D.A.</name></creator><creator><name>Dai Mi</name></creator><creator><name>Dimitriadis G.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Foley R.J.,Jha S.W.</name></creator><creator><name>Kelsey L.</name></creator><creator><name>Kirshner R.P.</name></creator><creator><name>Moller A.</name></creator><creator><name>Muir J.</name></creator><creator><name>Nadathur S.,Pan Y.-C.</name></creator><creator><name>Rest A.</name></creator><creator><name>Rojas-Bravo C.</name></creator><creator><name>Sako M.</name></creator><creator><name>Siebert M.R.</name></creator><creator><name>Smith M.,Stahl B.E.</name></creator><creator><name>Wiseman P.</name></creator><date role="Updated">2025-02-12T20:09:16Z</date><date role="Created">2024-10-21T14:07:52Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>supernovae</subject><subject>redshifted</subject><subject>photometry</subject><subject>visible-astronomy</subject><subject>surveys</subject><subject>astronomical-models</subject><description>We present constraints on cosmological parameters from the Pantheon+ analysis of 1701 light curves of 1550 distinct Type Ia supernovae (SNeIa) ranging in redshift from z=0.001 to 2.26. This work features an increased sample size from the addition of multiple cross-calibrated photometric systems of SNe covering an increased redshift span, and improved treatments of systematic uncertainties in comparison to the original Pantheon analysis, which together result in a factor of 2 improvement in cosmological constraining power. For a flat {Lambda}CDM model, we find {Omega}_M_=0.334+/-0.018 from SNe Ia alone. For a flat w_0_CDM model, we measure w_0_=-0.90+/-0.14 from SNeIa alone, H_0_=73.5+/-1.1km/s/Mpc when including the Cepheid host distances and covariance (SH0ES), and w_0_=-0.978_-0.031_^+0.024^ when combining the SN likelihood with Planck constraints from the cosmic microwave background (CMB) and baryon acoustic oscillations (BAO); both w_0_ values are consistent with a cosmological constant. We also present the most precise measurements to date on the evolution of dark energy in a flat w_0_w_a_CDM universe, and measure w_a_=-0.1_-2.0_^+0.9^ from Pantheon+ SNe Ia alone, H_0_=73.3+/-1.1km/s/Mpc when including SH0ES Cepheid distances, and w_a_=-0.65_-0.32_^+0.28^ when combining Pantheon+ SNe Ia with CMB and BAO data. Finally, we find that systematic uncertainties in the use of SNe Ia along the distance ladder comprise less than one-third of the total uncertainty in the measurement of H_0_ and cannot explain the present "Hubble tension" between local measurements and early universe predictions from the cosmological model.</description><source format="bibcode">2022ApJ...938..110B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/938/110</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/607/665">J/ApJ/607/665 : Type Ia supernovae at z&gt;1 discovered by HST (Riess+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/527">J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/700/331">J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/190/418">J/ApJS/190/418 : Light curves for 165 SNe (Ganeshalingam+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/523/A7">J/A+A/523/A7 : Light curves of type Ia supernovae in SNLS (Guy+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/566">J/ApJ/722/566 : Host galaxies of SNeIa in SDSS-II SN survey (Lampeitl+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/406/782">J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/PASP/122/1">J/PASP/122/1 : BVRI light curves of SN 2007gi (Zhang+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/529/L4">J/A+A/529/L4 : Reddening law of type Ia supernovae (Chotard+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/192/1">J/ApJS/192/1 : Light-curve parameters from the SNLS (Conley+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/738/162">J/ApJ/738/162 : SN Ia candidates from the SDSS-II SN Survey (Sako+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/200/12">J/ApJS/200/12 : CfA4: light curves for 94 type Ia SNe (Hicken+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/85">J/ApJ/746/85 : THe HST Cluster Supernova Survey. 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