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<ri:Resource created="2021-04-16T07:28:15Z" 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>GRB X-ray flare temporal and spectral properties</title><shortName>J/ApJ/884/59</shortName><identifier>ivo://CDS.VizieR/J/ApJ/884/59</identifier><altIdentifier>doi:10.26093/cds/vizier.18840059</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Liu C.</name></creator><creator><name>Mao J.</name></creator><date role="Updated">2021-07-05T11:09:35Z</date><date role="Created">2021-04-16T07:28:15Z</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>x-ray-sources</subject><subject>redshifted</subject><description>Gamma-ray bursts (GRBs) can be divided into three subclasses: X-ray flash (XRF), X-ray rich (XRR), and classical GRB (C-GRB). An X-ray flare is the rebrightening emission shown in the early X-ray afterglow of some GRBs. In this paper, we comprehensively examine the X-ray flare properties among XRF, XRR, and C-GRB subclasses. We utilize the XRF, XRR, and C-GRB subclass samples obtained from the Swift-BAT3 catalog, and the X-ray flare observational properties are collected from Falcone+ (2007ApJ...671.1921F), Chincarini+ (2010MNRAS.406.2113C), and Yi+ (2016, J/ApJS/224/20). We find that XRFs and XRRs have more bright X-ray flares than C-GRBs. The ratio of the X-ray flare fluence to the prompt emission fluence has different distributions between XRF and C-GRB subclasses. The linear correlation between the duration and the peak time of the X-ray flares is also different between XRF and C-GRB subclasses. We are inclined to identify the GRBs with the bright X-ray flares as XRFs or XRRs. We discuss some issues that are related to the XRF/XRR/C-GRB classification. We also caution the selection effects and the instrument bias in our investigation. Large samples are required in the future to further confirm our results.</description><source format="bibcode">2019ApJ...884...59L</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/884/59</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/B/swift">B/swift : Swift Master Catalog (HEASARC, 2004-)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/126/19">J/ApJS/126/19 : BATSE gamma-ray burst spectral catalog. I. (Preece+, 2000)</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/866/97">J/ApJ/866/97 : Swift X-ray flash &amp; rich gamma-ray bursts in BAT3 (Bi+, 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/884/59</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/884/59</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/884/59</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/884/59</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/884/59</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/884/59</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><capability xsi:type="cs:ConeSearch" standardID="ivo://ivoa.net/std/ConeSearch"><description>Cone search capability for table J/ApJ/884/59/table1 (Temporal properties of X-ray flares among X-ray flash (XRF), X-ray rich (XRR) and classical GRB (C-GRB))</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/884/59/table1?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/884/59/table1?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/884/59/table1?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>34.4675</ra><dec>-50.187725</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/186 205 207 314 462 500 550 699 877 908 918 1001 1882 2336 2793 3038 3405 3506 3536 3586 3589 3700 3935 4450 4485 5253 5606 6004 6404 7043 7356 7363 7532 7558 7589 7685 8021 8182 8798 8954 9024 9069 9321 9714 9827 9926 9989 10135 10407 10445 10680 10723 10852 10948 11140 11372 11456 12020 12134 12226 13312 13331 13558 13574 13787 13889 13898 14248 14555 14567 14846 14892 14977 15054 15320 15485 15498 15530 15613 15702 15820 15915 15995 16232 16292 16991 17279 17316 17453 17721 17814 17980 18258 18494 18728 18777 18910 18930 19049 19168 19731 20191 20360 20655 20668 21284 21903 21962 22559 22580 22624 23138 24007 24036 24041 25131 25293 25733 25901 25926 25946 26503 27085 27566 27933 28032 28033 28496 28726 28831 28863 29685 29731 29816 30088 30235 30553 30692 31028 31092 31143 31281 31385 31547 31700 31847 31934 32234 32676 33265 33278 33841 33977 34435 34461 34465 34590 34788 34832 34949 35045 35088 35256 35393 36066 36297 36528 37324 37383 37459 37675 37737 37830 38046 38504 38926 39076 39432 39881 39912 40167 40272 40433 40559 40778 41020 41989 42952 43193 43920 44419 44822 45008 45088 45402 45561 45729 45836 46395 46989 47162 47245 48189 48371 48422 48458 49034</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/884/59?format=ascii</footprint><waveband>Gamma-ray</waveband><waveband>X-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/ApJ/884/59/table1</name><description>Temporal properties of X-ray flares among X-ray flash (XRF), X-ray rich (XRR) and classical GRB (C-GRB)</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>GRB</name><description>GRB Name (YYMMDDA)</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>Type</name><description>GRB Type (1)</description><ucd>src.class</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>Int</name><description>GRB belongs to an intermediate class</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column><column><name>z</name><description>[0.25/8.3]? Redshift (2)</description><ucd>src.redshift</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>T90</name><description>[0.3/811]? Burst duration time (2)</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_T90</name><description>[0.03/560]? Uncertainty in T90 (2)</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Epa</name><description>[0.018/26]? GRB peak energy (2)</description><unit>100keV</unit><ucd>em.energy</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Epa</name><description>[5e-5/14.5]? Uncertainty in Epa (2)</description><unit>100keV</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>alphaPL</name><description>[0.9/2.6]? Power-law model fit slope (2)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_alphaPL</name><description>[0.02/0.5]? Uncertainty in alphaPL (2)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>alphaCPL</name><description>[-0.7/2.5]? Cut-off power-law model fit slope (2)</description><ucd>stat.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_alphaCPL</name><description>[0.019/3.6]? Uncertainty in alphaCPL (2)</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Sp25</name><description>[0.9/898]? 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