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<ri:Resource created="1999-02-27T12:09:49Z" 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>New SNR candidates in M31</title><shortName>J/A+AS/114/215</shortName><identifier>ivo://CDS.VizieR/J/A+AS/114/215</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Magnier E.A.</name></creator><creator><name>Prins S.</name></creator><creator><name>van Paradijs J.</name></creator><creator><name>Lewin W.H.G.</name></creator><creator><name>Supper R.,Hasinger G.</name></creator><creator><name>Pietsch W.</name></creator><creator><name>Truemper J.</name></creator><date role="Updated">1999-02-27T11:10:03Z</date><date role="Created">1999-02-27T12:09:49Z</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>supernova-remnants</subject><subject>h-ii-regions</subject><description>We have performed a CCD H{alpha}, [SII], V survey of ~1.0 square degree of the disk of M 31 to search for new supernova remnant (SNR) candidates. We have identified candidates based on a combination of criteria: optical line-flux ratios, the presence or absence of ionizing blue stars, and optical morphology. We have identified a total of 178 candidate SNRs, divided into three confidence categories: 13 with the highest confidence, 54 with moderate confidence, and 111 with the lowest confidence. We have also identified 14 large structures with the characteristics of the superbubbles seen in the Galaxy and Magellanic Clouds. Of our 178 candidates, 15 have been identified in previous searches (Braun &amp; Walterbos 1993; Blair et al. 1981; D'Odorico et al. 1980). We present finding charts of all candidate SNRs and the superbubbles we have noted. 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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>ID</name><description>Identification number</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>DeltaRA</name><description>Approximate extent of the object in right ascension</description><unit>arcsec</unit><ucd>phys.angSize;pos.eq.ra</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DeltaDE</name><description>Approximate extent of the object in declination</description><unit>arcsec</unit><ucd>phys.angSize;pos.eq.dec</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Diam</name><description>? Diameter of the object</description><unit>arcsec</unit><ucd>phys.angSize;src</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>n_Diam</name><description>When '*' extrapolated diameter</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Pict</name><description>Picture number</description><ucd>meta.id</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Fig</name><description>Figure number (5a through 5m)</description><ucd>meta.bib.fig</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Field</name><description>Field number in which the candidate was identified</description><ucd>obs.field</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Comments</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="81*">char</dataType></column></table><table><name>J/A+AS/114/215/table7</name><description>SNR candidates from other authors not identified in our images</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>ID</name><description>SNR Identification</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>RAJ2000</name><description>Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd></column><column><name>Comments</name><description>Comments</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="65*">char</dataType></column></table></schema></tableset></ri:Resource>