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<ri:Resource created="2015-03-27T07:03:57Z" status="active" updated="2025-05-19T09:50:00Z" version="1.2" 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/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>GRB 081007 and GRB 090424 light curves</title><shortName>J/ApJ/774/114</shortName><identifier>ivo://CDS.VizieR/J/ApJ/774/114</identifier><altIdentifier>doi:10.26093/cds/vizier.17740114</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Jin Z.-P.</name></creator><creator><name>Covino S.</name></creator><creator><name>Della Valle M.</name></creator><creator><name>Ferrero P.</name></creator><creator><name>Fugazza D.</name></creator><creator><name>Malesani D.,Melandri A.</name></creator><creator><name>Pian E.</name></creator><creator><name>Salvaterra R.</name></creator><creator><name>Bersier D.</name></creator><creator><name>Campana S.</name></creator><creator><name>Cano Z.,Castro-Tirado A.J.</name></creator><creator><name>D'Avanzo P.</name></creator><creator><name>Fynbo J.P.U.</name></creator><creator><name>Gomboc A.</name></creator><creator><name>Gorosabel J.,Guidorzi C.</name></creator><creator><name>Haislip J.B.</name></creator><creator><name>Hjorth J.</name></creator><creator><name>Kobayashi S.</name></creator><creator><name>LaCluyze A.P.,Marconi G.</name></creator><creator><name>Mazzali P.A.</name></creator><creator><name>Mundell C.G.</name></creator><creator><name>Piranomonte S.</name></creator><creator><name>Reichart D.E.,Sanchez-Ramirez R.</name></creator><creator><name>Smith R.J.</name></creator><creator><name>Steele I.A.</name></creator><creator><name>Tagliaferri G.</name></creator><creator><name>Tanvir N.R.,Valenti S.</name></creator><creator><name>Vergani S.D.</name></creator><creator><name>Vestrand T.</name></creator><creator><name>Walker E.S.</name></creator><creator><name>Wozniak P.</name></creator><date role="Updated">2017-06-26T11:48:57Z</date><date role="Created">2015-03-27T07:03:57Z</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><subject>infrared-photometry</subject><subject>visible-astronomy</subject><subject>broad-band-photometry</subject><subject>supernovae</subject><description>We discuss the results of the analysis of multi-wavelength data for the afterglows of GRB 081007 and GRB 090424, two bursts detected by Swift. One of them, GRB 081007, also shows a spectroscopically confirmed supernova, SN 2008hw, which resembles SN 1998bw in its absorption features, while the maximum magnitude may be fainter, up to 0.7mag, than observed in SN 1998bw. Bright optical flashes have been detected in both events, which allows us to derive solid constraints on the circumburst-matter density profile. This is particularly interesting in the case of GRB 081007, whose afterglow is found to be propagating into a constant-density medium, yielding yet another example of a gamma-ray burst (GRB) clearly associated with a massive-star progenitor which did not sculpt the surroundings with its stellar wind. There is no supernova component detected in the afterglow of GRB 090424, likely due to the brightness of the host galaxy, comparable to the Milky Way. We show that the afterglow data are consistent with the presence of both forward- and reverse-shock emission powered by relativistic outflows expanding into the interstellar medium. The absence of optical peaks due to the forward shock strongly suggests that the reverse-shock regions should be mildly magnetized. The initial Lorentz factor of outflow of GRB 081007 is estimated to be {Gamma}~200, while for GRB 090424 a lower limit of {Gamma}&gt;170 is derived. We also discuss the prompt emission of GRB 081007, which consists of just a single pulse. We argue that neither the external forward-shock model nor the shock-breakout model can account for the prompt emission data and suggest that the single-pulse-like prompt emission may be due to magnetic energy dissipation of a Poynting-flux-dominated outflow or to a dissipative photosphere.</description><source format="bibcode">2013ApJ...774..114J</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/774/114</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>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/565/A72">J/A+A/565/A72 : Opt. &amp; X-ray light curves of BAT6 sample (Melandri+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/557/A12">J/A+A/557/A12 : Optical light curves of {gamma}-ray bursts (Zaninoni+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/428/729">J/MNRAS/428/729 : GRB Swift X-ray light curves analysis (Margutti+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/20">J/ApJS/209/20 : Swift GRB catalog with X-ray data (Grupe+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/15">J/ApJ/763/15 : Fermi GRB analysis. 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(Kann+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/711/495">J/ApJ/711/495 : Durations of Swift/BAT GRBs (Butler+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/397/1177">J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009)</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/ApJ/774/114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/774/114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/774/114</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/774/114</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/774/114</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/774/114</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><coverage><spectral>2.762881831355591e-19 3.3785437584409506e-19</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Gamma-ray</waveband><waveband>Optical</waveband><waveband>Infrared</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/774/114/table1</name><description>Properties of GRB 081007 and GRB 090424</description><column><name>SN</name><description>SN detection</description><ucd>meta.id.assoc</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><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>GRB</name><description>GRB identifier (YYMMDD)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>LC</name><description>Light curves</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>T90</name><description>T_90_ duration</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_T90</name><description>? 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Rgal uncertainty</description><unit>mag</unit><ucd>stat.error;pos.distance;pos.galactocentric</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/774/114/table3</name><description>Optical observations of GRB 090424</description><column><name>l_mag</name><description>Limit flag on mag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Error in mag</description><unit>mag</unit><ucd>stat.error;phot.mag</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/ApJ/774/114/table2</name><description>Optical observations of GRB 081007</description><column><name>l_mag</name><description>Limit flag on mag</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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