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<ri:Resource created="2026-08-20T09:26:50Z" status="active" updated="2026-08-20T09:02:20Z" 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>HST photometry of SNe in nearby galaxies</title><shortName>J/ApJ/964/172</shortName><identifier>ivo://CDS.VizieR/J/ApJ/964/172</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Baer-Way R.</name></creator><creator><name>DeGraw A.</name></creator><creator><name>Zheng W.</name></creator><creator><name>Van Dyk S.D.</name></creator><creator><name>Filippenko A.V.</name></creator><creator><name>Fox O.D.,Brink T.G.</name></creator><creator><name>Kelly P.L.</name></creator><creator><name>Smith N.</name></creator><creator><name>Vasylyev S.S.</name></creator><creator><name>de Jaeger T.</name></creator><creator><name>Zhang K.,Stegman S.</name></creator><creator><name>Ross T.</name></creator><creator><name>Yunus S.</name></creator><date role="Updated">2026-08-20T09:02:20Z</date><date role="Created">2026-08-20T09:26:50Z</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>hst-photometry</subject><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><description>Over recent decades, robotic (or highly automated) searches for supernovae (SNe) have discovered several thousand events, many of them in quite nearby galaxies (distances &lt;30Mpc). Most of these SNe, including some of the best-studied events to date, were found before maximum brightness and have associated with them extensive follow-up photometry and spectroscopy. Some of these discoveries are so-called "SN impostors," thought to be superoutbursts of luminous blue variable stars, although possibly a new, weak class of massive-star explosions. We conducted a Snapshot program with the Hubble Space Telescope (HST) and obtained images of the sites of 31 SNe and four impostors, to acquire late-time photometry through two filters. The primary aim of this project was to reveal the origin of any lingering energy for each event, whether it is the result of radioactive decay or, in some cases, ongoing late-time interaction of the SN shock with preexisting circumstellar matter, or the presence of a light echo. Alternatively, lingering faint light at the SN position may arise from an underlying stellar population (e.g., a host star cluster, companion star, or a chance alignment). The results from this study complement and extend those from Snapshot programs by various investigators in previous HST cycles.</description><source format="bibcode">2024ApJ...964..172B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/964/172</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/B/hst">B/hst : HST Archived Exposures Catalog (STScI, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/408/181">J/MNRAS/408/181 : CN2002ch UBVRI and ugriz light curves (Pastorello+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/742/L18">J/ApJ/742/L18 : Follow-up photometry of SNIIb PTF 11eon (Arcavi+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/144/131">J/AJ/144/131 : Photometry and spectroscopy of SN 2010jl (Zhang+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/433/1871">J/MNRAS/433/1871 : UBVRI griz light curves of SN 2012aw (Bose+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/other/Nat/494.65">J/other/Nat/494.65 : SN 2010mc outburst before explosion (Ofek+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A17">J/A+A/562/A17 : SN 2011dh - The first 100 days (Ergon+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/781/42">J/ApJ/781/42 : Optical photometry of SN 2010jl (Ofek+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/215/9">J/ApJS/215/9 : PHAT X. 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