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<ri:Resource created="2019-06-27T07:31:22Z" 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>A VLA study of high-redshift GRBs. II. GRB140304A</title><shortName>J/ApJ/859/134</shortName><identifier>ivo://CDS.VizieR/J/ApJ/859/134</identifier><altIdentifier>doi:10.26093/cds/vizier.18590134</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Laskar T.</name></creator><creator><name>Berger E.</name></creator><creator><name>Margutti R.</name></creator><creator><name>Zauderer B.A.</name></creator><creator><name>Williams P.K.G.,Fong W.-F.</name></creator><creator><name>Sari R.</name></creator><creator><name>Alexander K.D.</name></creator><creator><name>Kamble A.</name></creator><date role="Updated">2024-09-05T20:09:26Z</date><date role="Created">2019-06-27T07:31:22Z</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>visible-astronomy</subject><subject>radio-continuum-emission</subject><description>We present detailed multifrequency, multiepoch radio observations of GRB 140304A at z=5.283 from 1 to 86GHz and from 0.45 to 89days. The radio and millimeter data exhibit unusual multiple spectral components, which cannot be simply explained by standard forward and reverse shock scenarios. Through detailed multiwavelength analysis spanning radio to X-rays, we constrain the forward shock parameters to E_k,iso_~4.9x10^54^erg, A_*_~2.6x10^-2^, {epsilon}_e_~2.5x10^-2^, {epsilon}_B_~5.9x10^-2^, p~2.6, and {theta}_jet_~1.1{deg}, yielding a beaming-corrected {gamma}-ray and kinetic energy, E_{gamma}_~2.3x10^49^erg and E_K_~9.5x10^50^erg, respectively. We model the excess radio emission as due to a combination of a late-time reverse shock (RS) launched by a shell collision, which also produces a rebrightening in the X-rays at ~0.26days, and either a standard RS or diffractive interstellar scintillation (ISS). Under the standard RS interpretation, we invoke consistency arguments between the forward and reverse shocks to derive a deceleration time, t_dec_~100s, the ejecta Lorentz factor, {Gamma}(t_dec_)~300, and a low RS magnetization, R_B_~0.6. Our observations highlight both the power of radio observations in capturing RS emission and thus constraining the properties of GRB ejecta and central engines and the challenge presented by ISS in conclusively identifying RS emission in GRB radio afterglows.</description><source format="bibcode">2018ApJ...859..134L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/859/134</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/MNRAS/397/1177">J/MNRAS/397/1177 : Swift-XRT observations of GRBs (Evans+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/560/A70">J/A+A/560/A70 : GRB 100621A unusual afterglow (Greiner+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/562/A29">J/A+A/562/A29 : GRB 100814A GROND and UVOT light curves (Nardini+, 2014)</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, 100901A multi-lambda obs. (Laskar+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/858/65">J/ApJ/858/65 : VLA study of high-redshift GRBs. I. GRB140311A (Laskar+, 2018)</relatedResource><relatedResource>http://www.swift.ac.uk/xrt_positions/00590206/ : Swift-XRT enhanced position</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/859/134</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/859/134</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/859/134</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/859/134</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/859/134</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/859/134</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><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Gamma-ray</waveband><waveband>Optical</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/859/134/table2</name><description>Swift UVOT observations of GRB 140304A</description><column><name>Filt</name><description>Swift/UVOT filter used</description><ucd>instr.setup;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">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>DeltaT</name><description>[0.003/6.7] Days since discovery on 2014 March 4 at 13:22:31 UT</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[9.5/409] The 3{sigma} flux density upper limit</description><unit>mJy</unit><ucd>phot.flux.density</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table><table><name>J/ApJ/859/134/table3</name><description>Optical observations of GRB 140304A</description><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>DeltaT</name><description>[0.0009/1.6] Time since discovery on 2014 March 4 at 13:22:31 UT</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tel</name><description>Observatory identifier ("HJT", "ICATE" or "NOT")</description><ucd>meta.id;instr.obsty</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Inst</name><description>Instrument identifier ("RATIR", "MASTER" or "ALFOSC")</description><ucd>meta.id;instr</ucd><dataType xsi:type="vs:VOTableType" arraysize="6*">char</dataType></column><column><name>Filt</name><description>Filter used (1)</description><ucd>instr.setup;instr.filter</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>Freq</name><description>[1.8e+14/4.6e+14] Midpoint frequency of Filt</description><unit>Hz</unit><ucd>em.freq</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>[0.002/0.8] Flux density in Filter (2)</description><unit>mJy</unit><ucd>phot.flux.density;em.opt</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[0.0008/0.2] Uncertainty in Flux (2)</description><unit>mJy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Det?</name><description>Detection?; 1=Yes</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Ref</name><description>GCN reference</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType" arraysize="79*">char</dataType></column></table><table><name>J/ApJ/859/134/table4</name><description>GRB 140304A: log of radio observations</description><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>DeltaT</name><description>[0.4/89.1] Days since discovery on 2014 March 4 at 13:22:31 UT</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Tel</name><description>Facility identifier ("VLA" or "CARMA")</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Freq</name><description>[1.4/85.5] Frequency of the radio observation</description><unit>GHz</unit><ucd>em.freq;obs</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>[0.02/1.2] Flux density at Freq</description><unit>mJy</unit><ucd>phot.flux.density;em.radio</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>e_Flux</name><description>[0.01/0.4] Uncertainty in Flux</description><unit>mJy</unit><ucd>stat.error;phot.flux</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Det?</name><description>Detection?; 1=Yes</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table></schema></tableset></ri:Resource>