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<ri:Resource created="2014-10-31T12:08:54Z" 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>SDSS-II supernovae Ia cosmological analysis</title><shortName>J/ApJ/763/88</shortName><identifier>ivo://CDS.VizieR/J/ApJ/763/88</identifier><altIdentifier>doi:10.26093/cds/vizier.17630088</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Campbell H.</name></creator><creator><name>D'Andrea C.B.</name></creator><creator><name>Nichol R.C.</name></creator><creator><name>Sako M.</name></creator><creator><name>Smith M.</name></creator><creator><name>Lampeitl H.,Olmstead M.D.</name></creator><creator><name>Bassett B.</name></creator><creator><name>Biswas R.</name></creator><creator><name>Brown P.</name></creator><creator><name>Cinabro D.</name></creator><creator><name>Dawson K.S.,Dilday B.</name></creator><creator><name>Foley R.J.</name></creator><creator><name>Frieman J.A.</name></creator><creator><name>Garnavich P.</name></creator><creator><name>Hlozek R.</name></creator><creator><name>Jha S.W.,Kuhlmann S.</name></creator><creator><name>Kunz M.</name></creator><creator><name>Marriner J.</name></creator><creator><name>Miquel R.</name></creator><creator><name>Richmond M.</name></creator><creator><name>Riess A.,Schneider D.P.</name></creator><creator><name>Sollerman J.</name></creator><creator><name>Taylor M.</name></creator><creator><name>Zhao G.-B.</name></creator><date role="Updated">2017-06-28T06:58:29Z</date><date role="Created">2014-10-31T12:08:54Z</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>surveys</subject><description>We present the cosmological analysis of 752 photometrically classified Type Ia Supernovae (SNe Ia) obtained from the full Sloan Digital Sky Survey II (SDSS-II) Supernova (SN) Survey, supplemented with host-galaxy spectroscopy from the SDSS-III Baryon Oscillation Spectroscopic Survey. Our photometric-classification method is based on the SN classification technique of Sako et al. (2011, Cat. J/ApJ/738/162), aided by host-galaxy redshifts (0.05&lt;z&lt;0.55). SuperNova ANAlysis simulations of our methodology estimate that we have an SN Ia classification efficiency of 70.8%, with only 3.9% contamination from core-collapse (non-Ia) SNe. We demonstrate that this level of contamination has no effect on our cosmological constraints. We quantify and correct for our selection effects (e.g., Malmquist bias) using simulations. When fitting to a flat {Lambda}CDM cosmological model, we find that our photometric sample alone gives {Omega}_m_=0.24^+0.07^_-0.05_ (statistical errors only). If we relax the constraint on flatness, then our sample provides competitive joint statistical constraints on {Omega}_m_ and {Omega}_{Lambda}_, comparable to those derived from the spectroscopically confirmed Three-year Supernova Legacy Survey (SNLS3). Using only our data, the statistics-only result favors an accelerating universe at 99.96% confidence. Assuming a constant wCDM cosmological model, and combining with H_0_, cosmic microwave background, and luminous red galaxy data, we obtain w=-0.96^+0.10^_-0.10_, {Omega}_m_=0.29^+0.02^_-0.02_, and {Omega}_k_=0.00^+0.03^_-0.02_ (statistical errors only), which is competitive with similar spectroscopically confirmed SNe Ia analyses. Overall this comparison is reassuring, considering the lower redshift leverage of the SDSS-II SN sample (z&lt;0.55) and the lack of spectroscopic confirmation used herein. These results demonstrate the potential of photometrically classified SN Ia samples in improving cosmological constraints.</description><source format="bibcode">2013ApJ...763...88C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/763/88</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/V/139">V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/568/A22">J/A+A/568/A22 : Joint analysis of SDSS-II and SNLS SNe Ia (Betoule+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/17">J/AJ/144/17 : SDSS &amp; CSP ugri phot. of 9 type Ia supernova (Mosher+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/143/126">J/AJ/143/126 : Nearby Type Ia supernovae spectroscopy (Blondin+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/755/125">J/ApJ/755/125 : Sample of SNe Ia with z&lt;0.25 from SDSS (Galbany+, 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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