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<ri:Resource created="2003-10-29T19:46:07Z" 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>TeV Gamma-Rays from 1ES1959+650</title><shortName>J/A+A/406/L9</shortName><identifier>ivo://CDS.VizieR/J/A+A/406/L9</identifier><altIdentifier>doi:10.26093/cds/vizier.34069009</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Aharonian F.</name></creator><creator><name>Akhperjanian A.</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 T.</name></creator><creator><name>Contreras J.L.</name></creator><creator><name>Cortina J.,Denninghoff S.</name></creator><creator/><creator><name>Fonseca M.V.</name></creator><creator><name>Girma M.</name></creator><creator><name>Goetting N.</name></creator><creator><name>Heinzelmann G.,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.</name></creator><creator><name>Kankanyan R.,Kestel M.</name></creator><creator><name>Kohnle A.</name></creator><creator><name>Konopelko A.</name></creator><creator><name>Kornmeyer H.</name></creator><creator><name>Kranich D.</name></creator><creator><name>Lampeitl H.,Lopez M.</name></creator><creator><name>Lorenz E.</name></creator><creator><name>Lucarelli F.</name></creator><creator><name>Mang O.</name></creator><creator><name>Meyer H.</name></creator><creator><name>Mirzoyan R.,Moralejo A.</name></creator><creator><name>Ona-Wilhelmi E.</name></creator><creator><name>Panter M.</name></creator><creator><name>Plyasheshnikov A.</name></creator><creator><name>Puehlhofer G.,delosReyes R.</name></creator><creator><name>Rhode W.</name></creator><creator><name>Ripken J.</name></creator><creator><name>Robrade J.</name></creator><creator><name>Rowell G.</name></creator><creator><name>Sahakian V.,Samorski M.</name></creator><creator><name>Schilling M.</name></creator><creator><name>Siems M.</name></creator><creator><name>Sobzynska D.</name></creator><creator><name>Stamm W.</name></creator><creator><name>Tluczykont M.,Vitale V.</name></creator><creator><name>Voelk H.J.</name></creator><creator><name>Wiedner C.A.</name></creator><creator><name>Wittek W.</name></creator><date role="Updated">2003-10-29T18:46:12Z</date><date role="Created">2003-10-29T19:46:07Z</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>bl-lacertae-objects</subject><description>TeV gamma-rays from the BL Lac object 1ES1959+650 have been measured during the years 2000 and 2001 with a significance of 5.2{sigma} at a value of 5.3% of the Crab flux and in May 2002 during strong outbursts with &gt;23{sigma} at a flux level of up to 2.2Crab, making 1ES1959+650 the TeV Blazar with the third best event statistics. The deep observation of 197.4h has been performed with the HEGRA stereoscopic system of 5 imaging atmospheric Cherenkov telescopes (IACT system). 1ES1959+650 is located at a redshift of z=0.047, providing an intermediate distance between the nearby Blazars Mkn 421 and Mkn 501, and the much more distant object H1426+428. This makes 1ES1959+650 an important candidate of the class of TeV Blazars in view of the absorption of TeV photons by the diffuse extragalactic background radiation (DEBRA). The differential energy spectrum of 1ES1959+650 during the flares can be well described by a power law with an exponential cut-off at (4.2(+0.8-0.6)_stat_+/-0.9_sys_) TeV and a spectral index of 1.83+/-0.15_stat_+/-0.08_sys_, while the low state spectrum can be fitted by a pure power law with a spectral index of 3.18+/-0.17_stat_+/-0.08_sys_.</description><source format="bibcode">2003A&amp;A...406L...9A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/406/L9</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/406/L9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/406/L9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/406/L9</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL use="base">https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/406/L9</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/406/L9</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/406/L9</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/406/L9/table4</name><description>Diurnal integral flux values of 1ES1959+650 above 2TeV from 2000 to 2002 as measured with the HEGRA stereoscopic system of 5 imaging atmospheric Cherenkov telescopes.</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>Mean MJD value (JD-2400000.5) of HEGRA observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>Duration</name><description>Duration of HEGRA observation</description><unit>h</unit><ucd>time.interval</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Flux</name><description>Integral flux above 2 TeV (1)</description><unit>1e-12cm**-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 integral flux above 2 TeV (1)</description><unit>1e-12cm**-2.s**-1</unit><ucd>stat.error</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>MJD1</name><description>Start MJD value of HEGRA observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>MJD2</name><description>End MJD value of HEGRA observation</description><unit>d</unit><ucd>time.epoch</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column></table></schema></tableset></ri:Resource>