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<ri:Resource created="2013-10-16T13:07:51Z" 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>Radio afterglow observations of GRBs</title><shortName>J/ApJ/746/156</shortName><identifier>ivo://CDS.VizieR/J/ApJ/746/156</identifier><altIdentifier>doi:10.26093/cds/vizier.17460156</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Chandra P.</name></creator><creator><name>Frail D.A.</name></creator><date role="Updated">2017-12-05T05:11:00Z</date><date role="Created">2013-10-16T13:07:51Z</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>radio-continuum-emission</subject><description>We present a catalog of radio afterglow observations of gamma-ray bursts (GRBs) over a 14 year period from 1997 to 2011. Our sample of 304 afterglows consists of 2995 flux density measurements (including upper limits) at frequencies between 0.6 GHz and 660 GHz, with the majority of data taken at 8.5 GHz frequency band (1539 measurements). We use this data set to carry out a statistical analysis of the radio-selected sample. The detection rate of radio afterglows has stayed unchanged almost at 31% before and after the launch of the Swift satellite. The canonical long-duration GRB radio light curve at 8.5 GHz peaks at three to six days in the source rest frame, with a median peak luminosity of 10^31^ erg/s/Hz. The peak radio luminosities for short-hard bursts, X-ray flashes, and the supernova-GRB classes are an order of magnitude or more fainter than this value. There are clear relationships between the detectability of a radio afterglow and the fluence or energy of a GRB, and the X-ray or optical brightness of the afterglow. However, we find few significant correlations between these same GRB and afterglow properties and the peak radio flux density. We also produce synthetic light curves at centimeter and millimeter bands using a range of blast wave and microphysics parameters derived from multiwavelength afterglow modeling, and we use them to compare to the radio sample. Finding agreement, we extrapolate this behavior to predict the centimeter and millimeter behavior of GRBs observed by the Expanded Very Large Array and the Atacama Large Millimeter Array.</description><source format="bibcode">2012ApJ...746..156C</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/746/156</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/ApJ/727/73">J/ApJ/727/73 : S/N composite spectrum of GRB afterglows (Christensen+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/195/2">J/ApJS/195/2 : The second Swift BAT GRB catalog (BAT2) (Sakamoto+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/720/1513">J/ApJ/720/1513 : The afterglows of Swift-era GRBs. I. (Kann+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/701/824">J/ApJ/701/824 : Afterglows of short and long-duration GRBs (Nysewander+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/690/163">J/ApJ/690/163 : The first Swift UV-Opt GRB afterglow catalog (Roming+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/180/192">J/ApJS/180/192 : BeppoSAX/GRBM {gamma}-ray Burst Catalog (Frontera+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/175/179">J/ApJS/175/179 : The BAT1 gamma-ray burst catalog (Sakamoto+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/686/1209">J/ApJ/686/1209 : Optical properties of GRB afterglows (Melandri+, 2008)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/455/813">J/A+A/455/813 : BeppoSAX catalog of GRB X-ray afterglows (De Pasquale+, 2006)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/609/935">J/ApJ/609/935 : Gamma-ray burst formation rate (Yonetoku+, 2004)</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/746/156</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/746/156</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/746/156</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/746/156</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/746/156</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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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>GRB</name><description>GRB name (YYMMDD)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType><flag>primary</flag></column><column><name>n_GRB</name><description>[m-r, ] Note(s) on GRB (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>R</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Inst</name><description>[A-T, sA] Instrument code (2)</description><ucd>meta.code;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>RAJ2000</name><description>[0,23] Hour of right ascension (J2000)</description><ucd>pos.eq.ra;meta.main</ucd></column><column><name>DEJ2000</name><description>[0,83] Degreee of declination (J2000)</description><ucd>pos.eq.dec;meta.main</ucd></column><column><name>X?</name><description>[XYN? ] X-ray afterglow detection? (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>O?</name><description>[XYN? ] Optical afterglow detection? (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>R?</name><description>[YN? ] Radio afterglow detection? (3)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Tel</name><description>Radio telescope (ATCA, EVLA or VLA)</description><ucd>instr.tel</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>n_Tel</name><description>[lr-v, ] Multiple observations (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>T90</name><description>[0.07,1800]? 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X-ray flux (0.3-10keV or 1.6-10keV) at 11hr in 10^-13^erg/cm^2^/s (5)</description><unit>1e-16W.m**-2</unit><ucd>phot.flux;em.X-ray</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>l_FR</name><description>Limit flag on FR</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>FR</name><description>[0.08,4328]? Optical R-band (0.7um) flux density at 11hr in {mu}Jy</description><unit>uJy</unit><ucd>phot.flux.density;em.opt.R</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>l_Tj</name><description>Limit flag on Tj</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Tj</name><description>[0.004/47.7]? 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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>GRB</name><description>GRB name (YYMMDDA)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Freq</name><description>[1.38,43] Frequency of the observation</description><unit>GHz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Fm</name><description>[50,59318] Peak flux density (F_m_) (1)</description><unit>uJy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Fm</name><description>[9,557]? Fm uncertainty</description><unit>uJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>tm</name><description>[1.3,179.1] Peak time (1)</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_tm</name><description>[0.1,11.3]? tm uncertainty</description><unit>d</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>tm/(1+z)</name><description>[0.6,97.6]? 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