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<ri:Resource created="2023-09-28T07:51:09Z" status="active" updated="2025-05-22T20:11:47Z" 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 emission of GRBs</title><shortName>J/ApJ/925/15</shortName><identifier>ivo://CDS.VizieR/J/ApJ/925/15</identifier><altIdentifier>doi:10.26093/cds/vizier.19250015</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Levine D.</name></creator><creator><name>Dainotti M.</name></creator><creator><name>Zvonarek K.J.</name></creator><creator><name>Fraija N.</name></creator><creator><name>Warren D.C.</name></creator><creator><name>Chandra P.,Lloyd-Ronning N.</name></creator><date role="Updated">2025-05-22T20:11:47Z</date><date role="Created">2023-09-28T07:51:09Z</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>gamma-ray-bursts</subject><subject>redshifted</subject><subject>astronomical-reference-materials</subject><subject>radio-sources</subject><description>Gamma-ray burst (GRB) afterglow emission can be observed from sub-TeV to radio wavelengths, though only 6.6% of observed GRBs present radio afterglows. We examine GRB radio light curves (LCs) to look for the presence of radio plateaus resembling the plateaus observed at X-ray and optical wavelengths. We analyze 404 GRBs from the literature with observed radio afterglow and fit 82 GRBs with at least five data points with a broken power-law model, requiring four parameters. From these, we find 18 GRBs that present a break feature resembling a plateau. We conduct the first multiwavelength study of the Dainotti correlation between the luminosity La and the rest-frame time of break Ta* for those 18 GRBs, concluding that the correlation exists and resembles the corresponding correlation at X-ray and optical wavelengths after correction for evolutionary effects. We compare Ta* for the radio sample with Ta* values in X-ray and optical data, finding significantly later break times in the radio. We propose that this late break time and the compatibility in slope suggest either a long-lasting plateau or the passage of a spectral break in the radio band. We also correct the distribution of the isotropic energy Eiso versus the rest-frame burst duration T*90 for evolutionary effects and conclude that there is no significant difference between the T*90 distributions for the radio LCs with a break and for those without.</description><source format="bibcode">2022ApJ...925...15L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/925/15</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/MNRAS/418/2202">J/MNRAS/418/2202 : Analysis of {gamma}-ray bursts (Dainotti+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/746/156">J/ApJ/746/156 : Radio afterglow observations of GRBs (Chandra+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/774/157">J/ApJ/774/157 : Swift GRBs with X-ray afterglows and z&lt;9.5 (Dainotti+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/781/37">J/ApJ/781/37 : Multi-band photometry of GRB 130427A (Perley+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/814/1">J/ApJ/814/1 : GRB 120326A, 100418A &amp; 100901A obs. (Laskar+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/806/52">J/ApJ/806/52 : 8 Fermi GRB afterglows follow-up (Singer+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/833/88">J/ApJ/833/88 : GRB 160509A VLA monitoring campain results (Laskar+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/850/161">J/ApJ/850/161 : Konus-Wind cat. of GRBs with z. I. (Tsvetkova+, 2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/65">J/ApJ/858/65 : A VLA study of high-z GRBs. I. GRB140311A (Laskar+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/473/1512">J/MNRAS/473/1512 : AMI 15.7GHz GRB catalogue (Anderson+, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/884/121">J/ApJ/884/121 : Radio to UV observations of GRB 181201A (Laskar+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/492/1919">J/MNRAS/492/1919 : Type I GRBs &amp; the new classification method (Minaev+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/893/77">J/ApJ/893/77 : A comprehensive statistical study of GRBs (Wang+, 2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/671/A116">J/A+A/671/A116 : GRB 210731A flux measurements (de Wet+, 2023)</relatedResource><relatedResource>http://www.mpe.mpg.de/~jcg/grbgen.html : Online collection of GRBs</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/925/15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/925/15</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/925/15</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/925/15</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/925/15</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/925/15</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/ApJ/925/15/table1 (82 GRBs used for fitting)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/925/15/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/925/15/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/925/15/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>105.6708</ra><dec>38.845</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/393 2336 3059 4450 4809 5004 5625 5840 6445 6729 8103 8733 9363 9910 9989 9998 10080 10589 11308 13312 13574 13720 15295 15320 15360 15595 16057 16187 16212 16276 16919 17038 17411 17911 19168 19519 19731 19864 20053 20679 21439 22008 22590 23413 24072 24779 24897 25131 25148 25336 26011 26365 26503 27961 28058 28063 28187 28344 28546 28555 30557 30886 31281 31583 32239 32646 35227 36074 36800 37123 39327 39594 40433 42545 43594 43853 44630 46488 47217 48388 48804 48968</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/925/15?format=ascii</footprint><waveband>Gamma-ray</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/925/15/table1</name><description>82 GRBs used for fitting</description><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>NED</name><description>NED column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">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>z</name><description>[0.0085/8] Spectroscopic redshift (1)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>T90</name><description>[1/1500] Rest-frame burst duration (1)</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>logFa</name><description>[13.6/17.4]? Log of flux at the end of the plateau emission; in erg/s/cm2 units</description><unit>log(mW.m**-2)</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_logFa</name><description>[0.01/0.4]? 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