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<ri:Resource created="2016-01-29T11:37:09Z" 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>Fermi/GBM GRB minimum timescales</title><shortName>J/ApJ/811/93</shortName><identifier>ivo://CDS.VizieR/J/ApJ/811/93</identifier><altIdentifier>doi:10.26093/cds/vizier.18110093</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Golkhou V.Z.</name></creator><creator><name>Butler N.R.</name></creator><creator><name>Littlejohns O.M.</name></creator><date role="Updated">2017-10-02T19:28:09Z</date><date role="Created">2016-01-29T11:37:09Z</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><subject>redshifted</subject><description>We constrain the minimum variability timescales for 938 gamma-ray bursts (GRBs) observed by the Fermi/Gamma-ray Burst Monitor instrument prior to 2012 July 11. The tightest constraints on progenitor radii derived from these timescales are obtained from light curves in the hardest energy channel. In the softer bands --or from measurements of the same GRBs in the hard X-rays from Swift-- we show that variability timescales tend to be a factor of two to three longer. Applying a survival analysis to account for detections and upper limits, we find median minimum timescale in the rest frame for long-duration and short-duration GRBs of 45 and 10ms, respectively. Less than 10% of GRBs show evidence for variability on timescales below 2ms. These shortest timescales require Lorentz factors &gt;~400 and imply typical emission radii R~1x10^14^cm for long-duration GRBs and R~3x10^13^cm for short-duration GRBs. We discuss implications for the GRB fireball model and investigate whether or not GRB minimum timescales evolve with cosmic time.</description><source format="bibcode">2015ApJ...811...93G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/811/93</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/J/ApJS/211/13">J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/431/3608">J/MNRAS/431/3608 : BeppoSAX/GRBM and Fermi/GBM long GRBs (Dichiara+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/763/15">J/ApJ/763/15 : Fermi GRB analysis. III. T_90_ distributions (Qin+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/748/134">J/ApJ/748/134 : Variability components in BATSE GRB LCs (Gao+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/756/112">J/ApJ/756/112 : Fermi/GBM GRB time-resolved spectral analysis (Lu+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/525/A53">J/A+A/525/A53 : GBM parameters for detected FERMI bursts (Guetta+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/520">J/ApJ/722/520 : Gamma-ray light curves of Fermi blazars (Abdo+, 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/268/305">J/MNRAS/268/305 : Variability of optically selected quasars (Hook+ 1994)</relatedResource><relatedResource>http://www.mpe.mpg.de/~jcg/grbgen.html : GRBs compilation</relatedResource><relatedResource>http://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html : Fermi</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/811/93</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/811/93</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/811/93</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/811/93</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/811/93</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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