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<ri:Resource created="2014-09-17T13:01:26Z" 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>Catalog of short gamma-ray transients</title><shortName>J/PAZh/40/271</shortName><identifier>ivo://CDS.VizieR/J/PAZh/40/271</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Minaev P.Yu.</name></creator><creator><name>Pozanenko A.S.</name></creator><creator><name>Molkov S.V.</name></creator><creator><name>Grebenev S.A.</name></creator><date role="Updated">2017-06-21T08:22:31Z</date><date role="Created">2014-09-17T13:01:26Z</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 analyzed the data obtained by the SPI telescope onboard the INTEGRAL observatory to search for short transient events with a duration from 1 ms to a few tens of seconds. An algorithm for identifying gamma-ray events against the background of a large number of charged particle interactions with the detector has been developed. The classification of events was made. Apart from the events associated with cosmic gamma-ray bursts (GRBs) confirmed by other space experiments and the activity of known soft gamma repeaters (for example, SGR 1806-20), previously unreported GRBs have been found. GRB candidates and short gamma-ray events probably associated with the activity of known SGRs and AXPs have been selected. The spectral evolution of 28 bright GRBs from the catalog has been studied extensively. A new method for investigating the spectral evolution is proposed. The energy dependence of the spectral lag for bursts with a simple structure of their light curves and for individual pulses of multipulse events is shown to be described by a logarithmic function, lag~Alog(E). It has been established that the parameter A depends on the pulse duration, with the dependence being universal for all of the investigated GRBs. No negative spectral lags have been detected for bursts with a simple structure of their light curves.</description><source format="bibcode">2014AstL...40..235M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/PAZh/40/271</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/528/A122">J/A+A/528/A122 : SwiftFT catalog (Puccetti+, 2011)</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/208/21">J/ApJS/208/21 : The BATSE 5B GRB spectral catalog (Goldstein+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/211/13">J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)</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/PAZh/40/271</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/PAZh/40/271</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/PAZh/40/271</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/PAZh/40/271</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/PAZh/40/271</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/PAZh/40/271</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/PAZh/40/271/table4 (Observed properties of the GRBs detected in the SPI/INTEGRAL experiment)</description><interface xsi:type="vs:ParamHTTP" role="std"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/conesearch/J/PAZh/40/271/table4?</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/conesearch/J/PAZh/40/271/table4?</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/conesearch/J/PAZh/40/271/table4?</mirrorURL><queryType>GET</queryType><resultType>text/xml+votable</resultType></interface><maxSR>180.0</maxSR><maxRecords>50000</maxRecords><verbosity>true</verbosity><testQuery><ra>74.3877111</ra><dec>20.4846939</dec><sr>0.005555555555555556</sr></testQuery></capability><coverage><spatial>6/3795 10411 10836 11008 12848 14563 15315 15739 20094 23585 24201 24219 26085 28849 29100 29225 29230 29318 29569 29862 29884 30203 30409 30557 32074 32239 32646 34816 35200 35485 37910 39327 41285 41467 42409 43101 44475 47397 48054</spatial><footprint ivo-id="ivo://ivoa.net/std/moc">https://cdsarc.cds.unistra.fr/viz-bin/moc/J/PAZh/40/271?format=ascii</footprint><waveband>Gamma-ray</waveband></coverage><tableset><schema><name>default</name><table><name>J/PAZh/40/271/SGRs</name><description>Bursts of Soft {gamma}-ray Repetears (SGR) detected in SPI/INTEGRAL experiment</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Significance (only in table7)</description><ucd>stat.fit.goodness</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table><table><name>J/PAZh/40/271/table4</name><description>Observed properties of the GRBs detected in the SPI/INTEGRAL experiment</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</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType><flag>primary</flag></column><column><name>n_GRB</name><description>? Note on GRB (1)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Time</name><description>The trigger time (UTC)</description><ucd>time.epoch</ucd><flag>nullable</flag></column><column><name>T90</name><description>Time Duration time covering 90% of the counts</description><unit>s</unit><ucd>time.duration</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_T90</name><description>rms uncertainty on T90</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>glow</name><description>[XOR ] Afterglow observation (X-ray, Optical, Radio)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="3*">char</dataType></column><column><name>lags</name><description>Spectral lag observations (tables 8 and 9)</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>RAJ2000</name><description>? Right ascension (J2000)</description><unit>deg</unit><ucd>pos.eq.ra;meta.main</ucd><flag>nullable</flag></column><column><name>DEJ2000</name><description>? Declination (J2000)</description><unit>deg</unit><ucd>pos.eq.dec;meta.main</ucd><flag>nullable</flag></column><column><name>l_ePos</name><description>Limit flag on ePos</description><ucd>meta.code.error</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>ePos</name><description>? Localization accuracy of the burst</description><unit>arcmin</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>r_ePos</name><description>[6/58]? Prigin of the localization (1)</description><ucd>meta.ref;pos.frame</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>Offset</name><description>[2.8/53.5]? Off-axis angle between the burst direction and the center of the SPI field of view</description><unit>deg</unit><ucd>instr.offset</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Simbad</name><description>Simbad column added by the CDS</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table><table><name>J/PAZh/40/271/table8</name><description>Spectral lag of the GRBs detected in the SPI/INTEGRAL experiment determined by the new method</description><column><name>GRB</name><description>GRB name</description><ucd>meta.id;meta.main</ucd><dataType xsi:type="vs:VOTableType" arraysize="7*">char</dataType></column><column><name>recno</name><description>Record number assigned by the VizieR team. 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Number of components in the GRB light curve used (1)</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>n_Nc</name><description>[fsv] Note on Nc (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="1*">char</dataType></column><column><name>Comp</name><description>Component (G1)</description><ucd>meta.code</ucd><dataType xsi:type="vs:VOTableType" arraysize="5*">char</dataType></column><column><name>n_Comp</name><description>[gp* ] Note on Comp (2)</description><ucd>meta.note</ucd><dataType xsi:type="vs:VOTableType" arraysize="2*">char</dataType></column><column><name>A1</name><description>Slope in the fit to the spectral lag-energy relation (3)</description><ucd>arith.grad;stat.fit.param;meta.modelled</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_A1</name><description>rms uncertainty on A1</description><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>A2</name><description>? 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Energy break (4)</description><unit>keV</unit><ucd>stat.fit.param</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Ebr</name><description>? rms uncertainty on Ebr</description><unit>keV</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>chi2</name><description>[0/9] {chi}^2^ value of the fit</description><ucd>stat.fit.chi2</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>dof</name><description>[6/20] Number of degrees of freedom</description><ucd>meta.number</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column></table><table><name>J/PAZh/40/271/table9</name><description>Spectral lag of the GRBs detected in the SPI/INTEGRAL experiment between the energy channels (25, 50), (50, 100), (100, 300), and (300, 1000) keV</description><column><name>recno</name><description>Record number assigned by the VizieR team. 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Spectral lag between energy channels (300-1000) and (25-50) keV</description><unit>s</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Lag4-1</name><description>? rms uncertainty on Lag4-1</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lag3-2</name><description>? Spectral lag between energy channels (100-300) and (50-100) keV</description><unit>s</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Lag3-2</name><description>? rms uncertainty on Lag3-2</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lag4-2</name><description>? Spectral lag between energy channels (300-1000) and (50-100) keV</description><unit>s</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Lag4-2</name><description>? rms uncertainty on Lag4-2</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>Lag4-3</name><description>? Spectral lag between energy channels (300-1000) and (100-300) keV</description><unit>s</unit><ucd>time;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column><column><name>e_Lag4-3</name><description>? rms uncertainty on Lag4-3</description><unit>s</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType><flag>nullable</flag></column></table></schema></tableset></ri:Resource>