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<ri:Resource created="1997-12-09T21:20:15Z" 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>Catalog of recent supernovae</title><shortName>J/ApJS/92/219</shortName><identifier>ivo://CDS.VizieR/J/ApJS/92/219</identifier><altIdentifier>doi:10.26093/cds/vizier.20920219</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>van den Bergh S.</name></creator><date role="Updated">2013-02-27T06:16:29Z</date><date role="Created">1997-12-09T21:20:15Z</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><description>A listing is given of all supernovae discovered between 1989 January 1 and 1993 April 1. The data show no evidence for a significant dependence of the discovery probability of supernovae on parent galaxy inclination to the line of sight. If no inclination corrections need to be applied, then the supernova rates in spirals are only about half as large as previously believed. The mean linear separation of supernovae of type II (SNe II) from the center of their parent galaxy increases with increasing distance (Shaw effect). The Shaw effect appears less evident, or absent, for (more luminous) supernovae of type Ia. The data are consistent with, but do not prove, the hypothesis that (presumably reddened) SNe II are more likely to be discovered in the red than in the blue. Due to intensive surveillance, most bright SNe Ia tend to be found before maximum, whereas the majority of faint SNe Ia are discovered after maximum light.</description><source format="bibcode">1994ApJS...92..219V</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/92/219</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/133">II/133 : Photoelectric UBV observations of supernovae</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/159">II/159 : Asiago Supernova Catalogue 1988</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/189">II/189 : A catalogue of magnitude observations of type I supernovae</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/201">II/201 : Sternberg SN Catalogue, 1994Sep.</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/205">II/205 : GCVS, Vol. V.: Extragalactic Variable Stars</relatedResource></relationship></content><rights>https://cds.unistra.fr/vizier-org/licences_vizier.html</rights><capability><interface xsi:type="vr:WebBrowser"><accessURL use="full">https://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/92/219</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/92/219</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/92/219</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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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>SN</name><description>Supernova name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>n_SN</name><description>[N] A 'N' indicates that it is not a supernova</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>MType</name><description>Parent galaxy classification types (2)</description><ucd>src.morph.type</ucd><dataType xsi:type="vs:VOTableType" arraysize="11*">char</dataType></column><column><name>RA1950</name><description>? Right ascension 1950</description><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DE1950</name><description>? Declination 1950</description><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>RV</name><description>? Radial velocity (3)</description><unit>km/s</unit><ucd>phys.veloc;pos.heliocentric</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Mag</name><description>? Discovered magnitude</description><unit>mag</unit><ucd>phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_Mag</name><description>Color of discovered magnitude (4)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>IAUC</name><description>? Number of IAU Circular giving discovery information</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Offsets</name><description>Offsets from nucleus of galaxy</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="9*">char</dataType></column><column><name>Type</name><description>Supernova type</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>IAUC(SN)</name><description>? Number of IAU Circular from which SN type was drawn</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Notes</name><description>? Remarks on some individual supernovae (5)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>_RA.icrs</name><description>Right ascension (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.ra</ucd><flag>nullable</flag><flag>indexed</flag></column><column><name>_DE.icrs</name><description>Declination (ICRS) (computed by VizieR, not part of the original data)</description><ucd>pos.eq.dec</ucd><flag>nullable</flag><flag>indexed</flag></column></table><table><name>J/ApJS/92/219/table2</name><description>Ages of supernova at discovery</description><column><name>recno</name><description>Record number assigned by the VizieR team. Should Not be used for identification.</description><ucd>meta.record</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>SN</name><description>Supernova name</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Gal</name><description>Parent galaxy name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Type</name><description>Type of the supernova</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>Age</name><description>Information on the spectral age</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="26*">char</dataType></column><column><name>l_T</name><description>[~&lt;] Limit flag on T</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>T</name><description>? 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