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<ri:Resource created="2017-10-03T16:14:21Z" 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>4.8GHz observations of SGR 1806-20</title><shortName>J/ApJ/634/L89</shortName><identifier>ivo://CDS.VizieR/J/ApJ/634/L89</identifier><altIdentifier>doi:10.26093/cds/vizier.16349089</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Gelfand J.D.</name></creator><creator><name>Lyubarsky Y.E.</name></creator><creator><name>Eichler D.</name></creator><creator><name>Gaensler B.M.</name></creator><creator><name>Taylor G.B.,Granot J.</name></creator><creator><name>Newton-McGee K.J.</name></creator><creator><name>Ramirez-Ruiz E.</name></creator><creator><name>Kouveliotou C.,Wijers R.A.M.J.</name></creator><date role="Updated">2017-11-03T14:06:57Z</date><date role="Created">2017-10-03T16:14:21Z</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>pulsars</subject><subject>gamma-ray-astronomy</subject><subject>radio-continuum-emission</subject><description>The 2004 December 27 giant {gamma}-ray flare detected from the magnetar SGR 1806-20 created an expanding radio nebula that we have monitored with the Australia Telescope Compact Array and the Very Large Array. These data indicate that there was an increase in the observed flux 25 days after the initial flare that lasted for 8 days, which we believe is the result of ambient material swept up and shocked by this radio nebula.</description><source format="bibcode">2005ApJ...634L..89G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/634/L89</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/634/L89</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/634/L89</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/634/L89</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/634/L89</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/634/L89</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/634/L89</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>3.180513520130092e-24 3.180513520130092e-24</spectral><footprint ivo-id="ivo://ivoa.net/std/moc"/><waveband>Gamma-ray</waveband><waveband>Radio</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/634/L89/table1</name><description>Radio observations at 4.8GHz of the radio nebula produced by SGR 1806-20</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>ObsDate</name><description>UT date of the average observational epoch</description><ucd>time.epoch;stat.mean</ucd><flag>nullable</flag></column><column><name>Day</name><description>[6.9/63] Days after Burst</description><unit>d</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Tel</name><description>Telescope used ("ATCA", 28 occurrences or "VLA")</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>S4.8GHz</name><description>[2.5/80] The 4.8GHz flux density (1)</description><unit>mJy</unit><ucd>phot.flux.density;em.radio.3-6GHz</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_S4.8GHz</name><description>[0.1/3] Uncertainty in S4.8GHz</description><unit>mJy</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column></table></schema></tableset></ri:Resource>