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<ri:Resource created="2026-02-16T09:21:02Z" status="active" updated="2026-03-02T20:03:36Z" 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-MDS supernovae classifications</title><shortName>J/ApJS/276/3</shortName><identifier>ivo://CDS.VizieR/J/ApJS/276/3</identifier><altIdentifier>doi:10.26093/cds/vizier/bb-8m-3</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Villar V.A.</name></creator><creator><name>Gomez S.</name></creator><creator><name>Berger E.</name></creator><creator><name>Gagliano A.</name></creator><date role="Updated">2026-03-02T20:03:36Z</date><date role="Created">2026-02-16T09:21:02Z</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>photometry</subject><subject>stellar-spectral-types</subject><description>With the advent of the Vera C. Rubin Observatory, the discovery rate of supernovae (SNe) will surpass the rate of SNe with real time spectroscopic follow-up by 3 orders of magnitude. Accurate photometric classifiers are essential to both select interesting events for follow-up in real time and for archival population-level studies. In this work, we investigate the impact of observable host-galaxy information on the classification of SNe, both with and without additional light-curve and redshift information. We find that host-galaxy information alone can successfully isolate relatively pure (&gt;90%) samples of Type Ia SNe with or without redshift information. With redshift information, we can additionally produce somewhat pure (&gt;70%) samples of Type II SNe and superluminous SNe. Additionally with redshift information, host- galaxy properties do not significantly improve the accuracy of SN classification when paired with complete light curves. In the absence of redshift information, however, galaxy properties significantly increase the accuracy of photometric classification. As a part of this analysis, we present the first formal application of a new objective function, the weighted hierarchical cross entropy, to the problem of SN classification. This objective function more naturally accounts for the hierarchical nature of SN classes and, more broadly, transients. Finally, we present a new set of SN classifications for the Pan-STARRS Medium Deep Survey of SNe that lack spectroscopic redshift, increasing the full photometric sample to &gt;4400 events.</description><source format="bibcode">2025ApJS..276....3V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/276/3</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/II/317">II/317 : The CFHTLS Survey (T0007 release) (Hudelot+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/412/1419">J/MNRAS/412/1419 : Nearby supernova rates (Leaman+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/424/2841">J/MNRAS/424/2841 : Morphology of supernova host galaxies (Habergham+, 2012)</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/ApJ/759/107">J/ApJ/759/107 : Core-collapse SNe and host galaxies (Kelly+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/7/107">J/ApJ/7/107 : Host galaxies of SNIa from SNfactory (Childress+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/905/93">J/ApJ/905/93 : Classif. of PS1-MDS SNe with Superphot (Hosseinzadeh+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/905/94">J/ApJ/905/94 : Classif. for PS1-MDS SNe with SuperRAENN (Villar+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/912/46">J/ApJ/912/46 : ZTF Type II supernovae with follow-up obs. (Bruch+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/255/29">J/ApJS/255/29 : PTF core-collapse SN host-galaxy sample. I. 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Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Name</name><description>Supernova name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>p(Ia)</name><description>[0/1] Probability of Type Ia classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(Ia)</name><description>[0/0.51] Uncertainty in p(Ia)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(CC)</name><description>[0/1] Probability of core-collapse classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(CC)</name><description>[0/0.51] Uncertainty in p(CC)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(H-rich)</name><description>[0/1] Probability of hydrogen-rich classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(H-rich)</name><description>[0/0.47] Uncertainty in p(H-rich)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(H-poor)</name><description>[0/1] Probability of hydrogen-poor classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(H-poor)</name><description>[0/0.48] Uncertainty in p(H-poor)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(SLSN)</name><description>[0/1] Probability of superluminous supernova classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(SLSN)</name><description>[0/0.45] Uncertainty in p(SLSN)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(II)</name><description>[0/0.91] Probability of Type II classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(II)</name><description>[0/0.39] Uncertainty in p(II)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(IIn)</name><description>[0/0.86] Probability of Type IIn classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(IIn)</name><description>[0/0.41] Uncertainty in p(IIn)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>p(Ibc)</name><description>[0/0.92] Probability of Type Ibc classification</description><ucd>meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_p(Ibc)</name><description>[0/0.42] Uncertainty in p(Ibc)</description><ucd>stat.error;meta.code.class;stat.probability</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>H20</name><description>Display data from Hosseinzadeh+ 2020, J/ApJ/905/93</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA</name><description>Positions from Villar+ 2020, J/ApJ/905/94 (right ascension part)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>_DE</name><description>Positions from Villar+ 2020, J/ApJ/905/94 (declination part)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column></table></schema></tableset></ri:Resource>