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<ri:Resource created="2016-05-31T12:44:40Z" 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>The cosmic TeV gamma-ray background spectrum</title><shortName>J/ApJ/818/187</shortName><identifier>ivo://CDS.VizieR/J/ApJ/818/187</identifier><altIdentifier>doi:10.26093/cds/vizier.18180187</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Inoue Y.</name></creator><creator><name>Tanaka Y.T.</name></creator><date role="Updated">2017-06-21T08:21:57Z</date><date role="Created">2016-05-31T12:44:40Z</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>active-galactic-nuclei</subject><description>The Fermi gamma-ray space telescope has revolutionized our understanding of the cosmic gamma-ray background radiation in the GeV band. However, investigation on the cosmic TeV gamma-ray background radiation still remains sparse. Here, we report the lower bound on the cosmic TeV gamma-ray background spectrum placed by the cumulative flux of individual detected extragalactic TeV sources including blazars, radio galaxies, and starburst galaxies. The current limit on the cosmic TeV gamma-ray background above 0.1TeV is obtained as 2.8x10^-8^(E/100GeV)^-0.55^exp(-E/2100GeV)[GeV/cm2/s/sr] &lt;E^2^dN/dE&lt;1.1x10^-7^(E/100GeV)^-0.49^[GeV/cm2/s/sr], where the upper bound is set by requirement that the cascade flux from the cosmic TeV gamma-ray background radiation can not exceed the measured cosmic GeV gamma-ray background spectrum. Two nearby blazars, Mrk421 and Mrk501, explain ~70% of the cumulative background flux at 0.8-4TeV, while extreme blazars start to dominate at higher energies. We also provide the cumulative background flux from each population, i.e., blazars, radio galaxies, and starburst galaxies which will be the minimum requirement for their contribution to the cosmic TeV gamma-ray background radiation.</description><source format="bibcode">2016ApJ...818..187I</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/818/187</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/ApJS/222/5">J/ApJS/222/5 : The second Fermi-LAT &gt;50GeV catalog (2FHL) (Ackermann+, 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/218/23">J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/799/86">J/ApJ/799/86 : Diffuse gamma-ray emission 0.1-820GeV (Ackermann+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/780/73">J/ApJ/780/73 : Redshifts of BL Lac objects from Fermi (Ajello+, 2014)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/207/16">J/ApJS/207/16 : BL Lac candidates for TeV observations (Massaro+, 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/542/A94">J/A+A/542/A94 : 1RXSJ101015.9-311909 VHE gamma-ray emission (HESS+, 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/722/520">J/ApJ/722/520 : Gamma-ray light curves of Fermi blazars (Abdo+, 2010)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/410/813">J/A+A/410/813 : 2001 Flare of Mkn 421 in gamma-ray (Aharonian+ 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/406/L9">J/A+A/406/L9 : TeV Gamma-Rays from 1ES1959+650 (Aharonian+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/390/39">J/A+A/390/39 : HEGRA AIROBICC gamma radiation above 15 TeV (Aharonian+, 2002)</relatedResource><relatedResource>http://tevcat.uchicago.edu/ : TeVCat online gamma-ray catalog</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/818/187</accessURL><mirrorURL title="VizieR at IUCAA: Pune, India">https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/818/187</mirrorURL><mirrorURL title="VizieR at SAAO: SAAO, South Africa">http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/818/187</mirrorURL></interface></capability><capability><interface xsi:type="vs:ParamHTTP"><accessURL 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