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<ri:Resource created="2017-05-22T12:01:13Z" 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>Limits on gamma-ray emission from galaxy clusters</title><shortName>J/ApJ/795/L21</shortName><identifier>ivo://CDS.VizieR/J/ApJ/795/L21</identifier><altIdentifier>doi:10.26093/cds/vizier.17959021</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Griffin R.D.</name></creator><creator><name>Dai X.</name></creator><creator><name>Kochanek C.S.</name></creator><date role="Updated">2017-06-12T08:59:28Z</date><date role="Created">2017-05-22T12:01:13Z</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>galaxy-clusters</subject><subject>galaxies</subject><subject>redshifted</subject><subject>gamma-ray-astronomy</subject><description>Galaxy clusters are predicted to produce {gamma}-rays through cosmic ray interactions and/or dark matter annihilation, potentially detectable by the Fermi Large Area Telescope (Fermi-LAT). We present a new, independent stacking analysis of Fermi-LAT photon count maps using the 78 richest nearby clusters (z&lt;0.12) from the Two Micron All Sky Survey cluster catalog. We obtain the lowest limit on the photon flux to date, 2.3x10^-11^ photons/cm2/s (95% confidence) per cluster in the 0.8-100 GeV band, which corresponds to a luminosity limit of 3.5x10^44^ photons/s. We also constrain the emission limits in a range of narrower energy bands. Scaling to recent cosmic ray acceleration and {gamma}-ray emission models, we find that cosmic rays represent a negligible contribution to the intra-cluster energy density and gas pressure.</description><source format="bibcode">2014ApJ...795L..21G</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/795/L21</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/VII/145">VII/145 : Nearby Galaxies Catalogue (NBG) (Tully 1988)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/110A">I/110A : Rich Clusters of Galaxies (Abell+ 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