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<ri:Resource created="2021-10-21T14:13:16Z" 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>{gamma}-ray emission of star-forming galaxies</title><shortName>J/ApJ/894/88</shortName><identifier>ivo://CDS.VizieR/J/ApJ/894/88</identifier><altIdentifier>doi:10.26093/cds/vizier.18940088</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Ajello M.</name></creator><creator><name>Di Mauro M.</name></creator><creator><name>Paliya V.S.</name></creator><creator><name>Garrappa S.</name></creator><date role="Updated">2022-01-19T13:04:51Z</date><date role="Created">2021-10-21T14:13:16Z</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>galaxies</subject><subject>infrared-sources</subject><subject>gamma-ray-astronomy</subject><description>A majority of the {gamma}-ray emission from star-forming galaxies is generated by the interaction of high-energy cosmic rays with the interstellar gas and radiation fields. Star-forming galaxies are expected to contribute to both the extragalactic {gamma}-ray background and the IceCube astrophysical neutrino flux. Using roughly 10yr of {gamma}-ray data taken by the Fermi Large Area Telescope, in this study we constrain the {gamma}-ray properties of star-forming galaxies. We report the detection of 11 bona fide {gamma}-ray-emitting galaxies and 2 candidates. Moreover, we show that the cumulative {gamma}-ray emission of below-threshold galaxies is also significantly detected at ~5{sigma} confidence. The {gamma}-ray luminosity of resolved and unresolved galaxies is found to correlate with the total (8-1000{mu}m) infrared luminosity as previously determined. Above 1GeV, the spectral energy distribution of resolved and unresolved galaxies is found to be compatible with a power law with a photon index of ~2.2-2.3. Finally, we find that star-forming galaxies account for roughly 5% and 3% of the extragalactic {gamma}-ray background and the IceCube neutrino flux, respectively.</description><source format="bibcode">2020ApJ...894...88A</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/894/88</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/274">VII/274 : The Roma BZCAT - 5th edition (Massaro+, 2015)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/112/315">J/ApJS/112/315 : Spectroscopic parameters of Seyfert nuclei (Ho+ 1997)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/143/377">J/ApJS/143/377 : UV-to-FIR magnitudes for 83 starburst galaxies (Wu+, 2002)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/AJ/126/1607">J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/A+A/465/71">J/A+A/465/71 : 21cm observations of 452 galaxies (Theureau+, 2007)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJS/184/230">J/ApJS/184/230 : Spitzer high-res. 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