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<ri:Resource created="2019-10-30T09:41:58Z" 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>Swift X-ray flash &amp; rich gamma-ray bursts in BAT3</title><shortName>J/ApJ/866/97</shortName><identifier>ivo://CDS.VizieR/J/ApJ/866/97</identifier><altIdentifier>doi:10.26093/cds/vizier.18660097</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Bi X.</name></creator><creator><name>Mao J.</name></creator><creator><name>Liu C.</name></creator><creator><name>Bai J.-M.</name></creator><date role="Updated">2019-10-30T13:53:15Z</date><date role="Created">2019-10-30T09:41:58Z</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>x-ray-sources</subject><description>We build a comprehensive sample to statistically describe the properties of X-ray flashes (XRFs) and X-ray riches (XRRs) from the third Swift Burst Alert Telescope (BAT3) catalog of Gamma-ray bursts (GRBs). We obtain 81 XRFs, 540 XRRs, and 394 classical GRBs (C-GRBs). We statistically explore the different properties of the {gamma}-ray prompt emission, the X-ray emission, the X-ray light-curve type, the association with supernovae (SNe), and the host galaxy properties for these sources. We confirm that most XRFs/XRRs are long GRBs with low values of peak energy E_peak_^obs^ and they are low-luminosity GRBs. XRFs, XRRs, and C-GRBs follow the same E_X,iso_-E_{gamma},iso_-E_peak,z_ correlations. Compared to the classical GRBs, XRFs are favorable to have the association with SN explosions. We do not find any significant differences of redshift distribution and host galaxy properties among XRFs, XRRs, and C-GRBs. We also discuss some observational biases and selection effects that may affect our statistical results. The GRB detectors with wide energy range and low energy threshold are expected for the XRF/XRR research in the future.</description><source format="bibcode">2018ApJ...866...97B</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/866/97</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/A+A/508/593">J/A+A/508/593 : GRB 080710 bright optical/NIR afterglow (Kruehler+, 2009)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/195/2">J/ApJS/195/2 : The second Swift BAT GRB catalog (BAT2) (Sakamoto+, 2011)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/209/20">J/ApJS/209/20 : Swift GRB catalog with X-ray data (Grupe+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/MNRAS/428/729">J/MNRAS/428/729 : GRB Swift X-ray light curves analysis (Margutti+, 2013)</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/ApJS/224/20">J/ApJS/224/20 : 10yr of Swift/XRT obs. of GRBs (Yi+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/826/45">J/ApJ/826/45 : GRB X-ray afterglows light curves analysis (Racusin+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/829/7">J/ApJ/829/7 : 3rd Swift/BAT GRB catalog (past ~11yrs) (BAT3) (Lien+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/852/53">J/ApJ/852/53 : Early X-ray flares in GRBs (Ruffini+, 2018)</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/866/97</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/866/97</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/866/97</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/866/97</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/866/97</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South 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Upper uncertainty in alphaCPL</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>S15-150</name><description>[0.1/10891]? Fluence of 15-150keV band in units of 10^-8^erg/cm^2^ (1)</description><unit>1e-08mJ.m**-2</unit><ucd>phot.fluence;em.gamma.hard</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_S15-150</name><description>[0.1/70]? Uncertainty in S15-150</description><unit>1e-08mJ.m**-2</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>SR</name><description>[0.7/54] Fluence ratio; 25-50keV/50-100keV</description><ucd>phot.fluence;arith.ratio</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_SR</name><description>[0.01/44]? 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