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<ri:Resource created="2006-12-17T17:51:21Z" 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>BeppoSAX catalog of GRB X-ray afterglows</title><shortName>J/A+A/455/813</shortName><identifier>ivo://CDS.VizieR/J/A+A/455/813</identifier><altIdentifier>doi:10.26093/cds/vizier.34550813</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>De Pasquale M.</name></creator><creator><name>Piro L.</name></creator><creator><name>Gendre B.</name></creator><creator><name>Amati L.</name></creator><creator><name>Antonelli L.A.</name></creator><creator><name>Costa E.,Feroci M.</name></creator><creator><name>Frontera F.</name></creator><creator><name>Nicastro L.</name></creator><creator><name>Soffitta P.</name></creator><creator><name>in't Zand J.</name></creator><date role="Updated">2006-12-17T16:52:03Z</date><date role="Created">2006-12-17T17:51:21Z</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>gamma-ray-astronomy</subject><subject>x-ray-sources</subject><description>We present the catalog of X-ray afterglow observed by BeppoSAX from the launch of the satellite to the end of the mission. Thirty-three X-ray afterglows out of 39 observations were securely identified based on their fading behavior. We have extracted the continuum parameters (decay index, spectral index, flux, absorption) for all available afterglows. 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