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<ri:Resource created="2003-12-28T23:01:54Z" 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>2001 Flare of Mkn 421 in gamma-ray</title><shortName>J/A+A/410/813</shortName><identifier>ivo://CDS.VizieR/J/A+A/410/813</identifier><altIdentifier>doi:10.26093/cds/vizier.34100813</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Aharonian F.A.</name></creator><creator><name>Akhperjanian A.G.</name></creator><creator><name>Beilicke M.</name></creator><creator><name>Bernloehr K.</name></creator><creator><name>Boerst H.-G.,Bojahr H.</name></creator><creator><name>Bolz O.</name></creator><creator><name>Coarasa J.A.</name></creator><creator><name>Contreras J.L.</name></creator><creator><name>Cortina J.,Denninghoff S.</name></creator><creator><name>Fonseca M.V.</name></creator><creator><name>Girma M.</name></creator><creator><name>Goebel F.</name></creator><creator><name>Goetting N.,Heinzelmann G.</name></creator><creator><name>Hermann G.</name></creator><creator><name>Heusler A.</name></creator><creator><name>Hofmann W.</name></creator><creator><name>Horns D.</name></creator><creator><name>Jung I.,Kankanyan R.</name></creator><creator><name>Kestel M.</name></creator><creator><name>Kettler J.</name></creator><creator><name>Kohnle A.</name></creator><creator><name>Konopelko A.</name></creator><creator><name>Kranich D.,Krawczynski H.</name></creator><creator><name>Lampeitl H.</name></creator><creator><name>Lopez M.</name></creator><creator><name>Lorenz E.</name></creator><creator><name>Lucarelli F.</name></creator><creator><name>Mang O.,Meyer H.</name></creator><creator><name>Mirzoyan R.</name></creator><creator><name>Moralejo A.</name></creator><creator><name>Ona-Wilhelmi E.</name></creator><creator><name>Paneque D.,Panter M.</name></creator><creator><name>Plyasheshnikov A.</name></creator><creator><name>Puehlhofer G.</name></creator><creator><name>de los Reyes R.</name></creator><creator><name>Rhode W.,Ripken J.</name></creator><creator><name>Rowell G.P.</name></creator><creator><name>Sahakian V.</name></creator><creator><name>Samorski M.</name></creator><creator><name>Schilling M.,Schweizer T.</name></creator><creator><name>Sevilla I.</name></creator><creator><name>Siems M.</name></creator><creator><name>Sobczynska D.</name></creator><creator><name>Stamm W.</name></creator><creator><name>Tluczykont M.,Tonello N.</name></creator><creator><name>Vitale V.</name></creator><creator><name>Voelk H.J.</name></creator><creator><name>Wagner R.M.</name></creator><creator><name>Wiedner C.A.,W.Wittek.</name></creator><date role="Updated">2003-12-28T22:02:41Z</date><date role="Created">2003-12-28T23:01:54Z</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>active-galactic-nuclei</subject><subject>bl-lacertae-objects</subject><subject>gamma-ray-astronomy</subject><description>In the first months of 2001 the AGN Mkn 421 showed highly variable, strong TeV activity at flux levels frequently exceeding 1 Crab. Here we present the light curve and energy spectrum of Mkn 421 as measured with the HEGRA stand alone telescope CT1. Around 30% of the data were taken under moonlight conditions. The spectrum shows a significant exponential energy cutoff at around 3.4 TeV. The results from the dark night- and the moon data are in excellent agreement with each other. A significant spectral shape variation depending on the flux level has been found. The TeV light curve is also found to be highly correlated with the X-ray light curve of the RXTE/ASM satellite, showing no significant time lag larger than 0.2d. The derived correlation coefficient of 0.83 corresponds to a 5.2{sigma} significance.</description><source format="bibcode">2003A&amp;A...410..813A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/410/813</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</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/A+A/410/813</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/410/813</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/410/813</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/410/813</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/410/813</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/410/813</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/A+A/410/813/table4</name><description>Integral flux values of Mkn 421</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>MJD</name><description>Modified Julian Date (MJD=JD-2400000.5)</description><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Flux</name><description>Integral Flux above 1 TeV (1)</description><unit>1e-11cm**-2.s**-1</unit><ucd>phot.flux.density;em.gamma.soft</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_Flux</name><description>error on the Integral Flux (1)</description><unit>1e-11cm**-2.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>ExpTime</name><description>observation time</description><unit>h</unit><ucd>time.duration;obs.exposure</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>HV</name><description>HV setting of the PMTs (2)</description><ucd>instr.setup</ucd><dataType xsi:type="vs:VOTableType" arraysize="4*">char</dataType></column></table></schema></tableset></ri:Resource>