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<ri:Resource created="2015-11-30T12:20:04Z" status="active" updated="2025-05-19T09:50:00Z" 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>PS1 SNe Ia (0.02&lt;z&lt;0.7) griz light curves</title><shortName>J/ApJ/795/44</shortName><identifier>ivo://CDS.VizieR/J/ApJ/795/44</identifier><altIdentifier>doi:10.26093/cds/vizier.17950044</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Rest A.</name></creator><creator><name>Scolnic D.</name></creator><creator><name>Foley R.J.</name></creator><creator><name>Huber M.E.</name></creator><creator><name>Chornock R.</name></creator><creator><name>Narayan G.,Tonry J.L.</name></creator><creator><name>Berger E.</name></creator><creator><name>Soderberg A.M.</name></creator><creator><name>Stubbs C.W.</name></creator><creator><name>Riess A.,Kirshner R.P.</name></creator><creator><name>Smartt S.J.</name></creator><creator><name>Schlafly E.</name></creator><creator><name>Rodney S.</name></creator><creator><name>Botticella M.T.,Brout D.</name></creator><creator><name>Challis P.</name></creator><creator><name>Czekala I.</name></creator><creator><name>Drout M.</name></creator><creator><name>Hudson M.J.</name></creator><creator><name>Kotak R.,Leibler C.</name></creator><creator><name>Lunnan R.</name></creator><creator><name>Marion G.H.</name></creator><creator><name>McCrum M.</name></creator><creator><name>Milisavljevic D.,Pastorello A.</name></creator><creator><name>Sanders N.E.</name></creator><creator><name>Smith K.</name></creator><creator><name>Stafford E.</name></creator><creator><name>Thilker D.</name></creator><creator><name>Valenti S.,Wood-Vasey W.M.</name></creator><creator><name>Zheng Z.</name></creator><creator><name>Burgett W.S.</name></creator><creator><name>Chambers K.C.</name></creator><creator><name>Denneau L.,Draper P.W.</name></creator><creator><name>Flewelling H.</name></creator><creator><name>Hodapp K.W.</name></creator><creator><name>Kaiser N.</name></creator><creator><name>Kudritzki R.-P.,Magnier E.A.</name></creator><creator><name>Metcalfe N.</name></creator><creator><name>Price P.A.</name></creator><creator><name>Sweeney W.</name></creator><creator><name>Wainscoat R.</name></creator><creator><name>Waters C.</name></creator><date role="Updated">2020-08-06T16:12:02Z</date><date role="Created">2015-11-30T12:20:04Z</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>surveys</subject><subject>redshifted</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>We present griz_P1_ light curves of 146 spectroscopically confirmed Type Ia supernovae (SNe Ia; 0.03&lt;z&lt;0.65) discovered during the first 1.5yr of the Pan-STARRS1 Medium Deep Survey. The Pan-STARRS1 natural photometric system is determined by a combination of on-site measurements of the instrument response function and observations of spectrophotometric standard stars. We find that the systematic uncertainties in the photometric system are currently 1.2% without accounting for the uncertainty in the Hubble Space Telescope Calspec definition of the AB system. A Hubble diagram is constructed with a subset of 113 out of 146 SNe Ia that pass our light curve quality cuts. The cosmological fit to 310 SNe Ia (113 PS1 SNe Ia + 222 light curves from 197 low-z SNe Ia), using only supernovae (SNe) and assuming a constant dark energy equation of state and flatness, yields {omega}=-1.120_-0.206_^+0.360^(Stat)_-0.291_^+0.269^(Sys). When combined with BAO+CMB(Planck)+H_0_, the analysis yields {Omega}_M_=0.280_-0.012_^+0.013^ and {omega}=-1.166_-0.069_^+0.072^ including all identified systematics. The value of w is inconsistent with the cosmological constant value of -1 at the 2.3{sigma} level. Tension endures after removing either the baryon acoustic oscillation (BAO) or the H_0_ constraint, though it is strongest when including the H_0_ constraint. If we include WMAP9 cosmic microwave background (CMB) constraints instead of those from Planck, we find {omega}=-1.124_-0.065_^+0.083^, which diminishes the discord to &lt;2{sigma}. We cannot conclude whether the tension with flat {Lambda}CDM is a feature of dark energy, new physics, or a combination of chance and systematic errors. The full Pan-STARRS1 SN sample with ~three times as many SNe should provide more conclusive results.</description><source format="bibcode">2014ApJ...795...44R</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/795/44</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/B/sn">B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/437/656">J/MNRAS/437/656 : SN PS1-11ap light curves (McCrum+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/433/2240">J/MNRAS/433/2240 : SALT2 param. and distances for SNe (Ganeshalingam+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/769/39">J/ApJ/769/39 : SNIbn PS1-12sk optical and NIR light curves (Sanders+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/552/A124">J/A+A/552/A124 : SNLS &amp; SDSS SN surveys phot. calibration (Betoule+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/88">J/ApJ/763/88 : SDSS-II SNe Ia cosmological analysis (Campbell+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/544/A81">J/A+A/544/A81 : Supernovae and their hosts in the SDSS DR8 (Hakobyan+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/538/A120">J/A+A/538/A120 : A unified supernova catalogue (Lennarz+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/425/1789">J/MNRAS/425/1789 : Berkeley supernova Ia program. 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