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<ri:Resource created="2007-10-25T10:21:23Z" 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>GRB from RICE data</title><shortName>J/other/APh/26.3</shortName><identifier>ivo://CDS.VizieR/J/other/APh/26.367</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Besson D.</name></creator><creator><name>Razzaque S.</name></creator><creator><name>Adams J.</name></creator><creator><name>Harris P.</name></creator><date role="Updated">2007-10-25T10:25:04Z</date><date role="Created">2007-10-25T10:21:23Z</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><description>We present limits on ultra-high energy (UHE; E_{nu}_&gt;10^15^eV) neutrino fluxes from gamma-ray bursts (GRBs), based on recently presented data, limits, and simulations from the RICE experiment. We use data from five recorded transients with sufficient photon spectral shape and redshift information to derive an expected neutrino flux, assuming that the observed photons are linked to neutrino production through pion decay via the well-known Waxman-Bahcall prescription. Knowing the declination of the observed burst, as well as the RICE sensitivity as a function of polar angle and the previously published non-observation of any neutrino events allows an estimate of the sensitivity to a given neutrino flux. Although several orders of magnitude weaker than the expected fluxes, our GRB neutrino flux limits are nevertheless the first in the PeVEeV energy regime. For completeness, we also provide a listing of other bursts, recorded at times when the RICE experiment was active, but requiring some assumptions regarding luminosity and redshift to permit estimates of the neutrino flux.</description><source format="bibcode">2007APh....26..367B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/APh/26.367</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/IX/20">IX/20 : The Fourth BATSE Burst Revised Catalog (Paciesas+ 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/IX/36">IX/36 : GRANAT/PHEBUS catalog of cosmic GRB (Terekhov+, 1994-2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+AS/129/1">J/A+AS/129/1 : GRANAT/WATCH catalogue of gamma-ray bursts (Sazonov+ 1998)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/120/399">J/ApJS/120/399 : ULYSSES supplement to GRB 3B catalog (Hurley+, 1999)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/134/385">J/ApJS/134/385 : Supplement to the BATSE GRB catalogs (Kommers+, 2001)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/427/87">J/A+A/427/87 : List of GRBs (Gorosabel+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/156/217">J/ApJS/156/217 : IPN supplement to BATSE untriggered GRBs (Hurley+, 2005)</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></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/other/APh/26.367</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/other/APh/26.367</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/other/APh/26.367</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/other/APh/26.367</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/other/APh/26.367</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/other/APh/26.367</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></coverage><tableset><schema><name>default</name><table><name>J/other/APh/26.367/appen</name><description>GRBs recorded in southern hemisphere, with incomplete spectral or redshift information</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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