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<ri:Resource created="2009-03-13T15:15:09Z" 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>Gamma-ray bursts with known redshifts</title><shortName>J/PAZh/35/10</shortName><identifier>ivo://CDS.VizieR/J/PAZh/35/10</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Badjin D.A.</name></creator><creator><name>Beskin G.M.</name></creator><creator><name>Greco G.</name></creator><date role="Updated">2017-06-27T06:38:35Z</date><date role="Created">2009-03-13T15:15:09Z</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>gamma-ray-astronomy</subject><description>Observational parameters of the optical and gamma-ray emissions from 58 gamma-ray bursts (GRBs) with discovered afterglows and known redshifts are analyzed. The distributions of these parameters and pair correlations between them are studied. Approximately half of the objects exhibit a relatively slow decrease in the optical flux at initial afterglow phases (with a power-law index in the decay law {alpha}&lt;1). Correlations have been found between the luminosities, energies, and durations of the optical and gamma-ray emissions, which can be explained by the presence of universal features in the light curves. A correlation of the peak luminosity for afterglows with the redshift and an anticorrelation of their durations with the redshift have been found for the first time. Against the background of a weak z dependence of the total afterglow energy, this effect can be explained by cosmological evolution of the GRB environment, which determines the rate of optical energy release.</description><source format="bibcode">2009PAZh...35...10B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/35/10</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/IX/20">IX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/36">IX/36 : GRANAT/PHEBUS catalog of cosmic GRB (Terekhov+, 1994-2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/1">J/A+AS/129/1 : GRANAT/WATCH catalogue of gamma-ray bursts (Sazonov+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/126/19">J/ApJS/126/19 : BATSE gamma-ray burst spectral catalog. I. (Preece+, 2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/134/385">J/ApJS/134/385 : Supplement to the BATSE GRB catalogs (Kommers+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/616/1072">J/ApJ/616/1072 : The GUSBAD catalog of gamma-ray bursts (Schmidt+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/438/1175">J/A+A/438/1175 : First INTEGRAL SPI-ACS Gamma-Ray Burst Catalogue (Rau+, 2005)</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/PAZh/35/10</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/35/10</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/35/10</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PAZh/35/10</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PAZh/35/10</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PAZh/35/10</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface></capability><capability standardID="ivo://ivoa.net/std/TAP#aux"><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://tapvizier.cds.unistra.fr/TAPVizieR/tap</accessURL></interface></capability><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/PAZh/35/10/tables (Parameters of the "observed" and "intrinsic" sample)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PAZh/35/10/tables?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/PAZh/35/10/tables?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PAZh/35/10/tables?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>75.4445833</ra><dec>11.7813889</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/393 500 557 3536 5726 6141 6258 7650 8103 9363 9910 9998 10080 10447 10589 11008 12597 13312 13924 17038 17453 17911 18030 18978 19519 19731 19864 20030 22008 23138 23413 24072 24993 25146 25148 25452 25901 27841 28058 28344 28546 31385 31494 31934 32239 33735 37123 39427 40433 40784 41095 43853 45008 45347 45938 47459 48804 49004</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PAZh/35/10?format=ascii</footprint><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/PAZh/35/10/tables</name><description>Parameters of the "observed" and "intrinsic" sample</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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