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<ri:Resource created="2011-03-07T13:28:09Z" 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 SNe survey: search and follow-up</title><shortName>J/AJ/135/348</shortName><identifier>ivo://CDS.VizieR/J/AJ/135/348</identifier><altIdentifier>doi:10.26093/cds/vizier.51350348</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Sako M.</name></creator><creator><name>Bassett B.</name></creator><creator><name>Becker A.</name></creator><creator><name>Cinabro D.</name></creator><creator><name>Dejongh F.</name></creator><creator><name>Depoy D.L.,Dilday B.</name></creator><creator><name>Doi M.</name></creator><creator><name>Frieman J.A.</name></creator><creator><name>Garnavich P.M.</name></creator><creator><name>Hogan C.J.</name></creator><creator><name>Holtzman J.,Jha S.</name></creator><creator><name>Kessler R.</name></creator><creator><name>Konishi K.</name></creator><creator><name>Lampeitl H.</name></creator><creator><name>Marriner J.</name></creator><creator><name>Miknaitis G.,Nichol R.C.</name></creator><creator><name>Prieto J.L.</name></creator><creator><name>Riess A.G.</name></creator><creator><name>Richmond M.W.</name></creator><creator><name>Romani R.,Schneider D.P.</name></creator><creator><name>Smith M.</name></creator><creator><name>Subbarao M.</name></creator><creator><name>Takanashi N.</name></creator><creator><name>Tokita K.,van der Heyden K.</name></creator><creator><name>Yasuda N.</name></creator><creator><name>Zheng C.</name></creator><creator><name>Barentine J.</name></creator><creator><name>Brewington H.,Choi C.</name></creator><creator><name>Dembicky J.</name></creator><creator><name>Harnavek M.</name></creator><creator><name>Ihara Y.</name></creator><creator><name>Im M.</name></creator><creator><name>Ketzeback W.,Kleinman S.J.</name></creator><creator><name>Krzesinski J.</name></creator><creator><name>Long D.C.</name></creator><creator><name>Malanushenko E.</name></creator><creator><name>Malanushenko V.,McMillan R.J.</name></creator><creator><name>Morokuma T.</name></creator><creator><name>Nitta A.</name></creator><creator><name>Pan K.</name></creator><creator><name>Saurage G.</name></creator><creator><name>Snedden S.A.</name></creator><date role="Updated">2017-06-26T11:49:33Z</date><date role="Created">2011-03-07T13:28:09Z</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>spectroscopy</subject><subject>surveys</subject><description>The Sloan Digital Sky Survey-II Supernova Survey has identified a large number of new transient sources in a 300deg^2^ region along the celestial equator during its first two seasons of a three-season campaign. Multi-band (ugriz) light curves were measured for most of the sources, which include solar system objects, galactic variable stars, active galactic nuclei, supernovae (SNe), and other astronomical transients. The imaging survey is augmented by an extensive spectroscopic follow-up program to identify SNe, measure their redshifts, and study the physical conditions of the explosions and their environment through spectroscopic diagnostics. During the survey, light curves are rapidly evaluated to provide an initial photometric type of the SNe, and a selected sample of sources are targeted for spectroscopic observations. In the first two seasons, 476 sources were selected for spectroscopic observations, of which 403 were identified as SNe. For the type Ia SNe, the main driver for the survey, our photometric typing and targeting efficiency is 90%. Only 6% of the photometric SN Ia candidates were spectroscopically classified as non-SN Ia instead, and the remaining 4% resulted in low signal-to-noise, unclassified spectra.</description><source format="bibcode">2008AJ....135..348S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/135/348</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/II/256">II/256 : Sternberg Supernova Catalogue, 2004 version (Tsvetkov+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/131/527">J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/659/122">J/ApJ/659/122 : Improved distances to type Ia supernovae (Jha+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/666/674">J/ApJ/666/674 : ESSENCE supernova survey (Miknaitis+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/135/1766">J/AJ/135/1766 : Sloan Digital Sky Survey-II supernova survey (Zheng+, 2008)</relatedResource><relatedResource>http://www.cfa.harvard.edu/supernova : The CfA SN Group home page</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/AJ/135/348</accessURL><mirrorURL title="VizieR at IUCAA: Pune, 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