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<ri:Resource created="2023-10-03T14:17:03Z" status="active" updated="2026-03-04T20:02:53Z" 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>Anomalous gamma-ray excess emissions</title><shortName>J/other/NatAs/2.</shortName><identifier>ivo://CDS.VizieR/J/other/NatAs/2.387</identifier><altIdentifier>doi:10.26093/cds/vizier/dt/ckdih</altIdentifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Macias O.</name></creator><creator><name>Gordon C.</name></creator><creator><name>Crocker R.M.</name></creator><creator><name>Coleman B.</name></creator><creator><name>Paterson D.</name></creator><creator><name>Horiuchi S.,Pohl M.</name></creator><date role="Updated">2026-03-04T20:02:53Z</date><date role="Created">2023-10-03T14:17:03Z</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>galactic-center</subject><subject>gamma-ray-astronomy</subject><description>An anomalous gamma-ray excess emission has been found in the Fermi Large Area Telescope data covering the centre of the Galaxy. Several theories have been proposed for this "Galactic centre excess". They include self-annihilation of dark-matter particles, an unresolved population of millisecond pulsars, an unresolved population of young pulsars, or a series of burst events. Here, we report on an analysis that exploits hydrodynamical modelling to register the position of interstellar gas associated with diffuse Galactic gamma-ray emission. We find evidence that the Galactic centre excess gamma rays are statistically better described by the stellar over-density in the Galactic bulge and the nuclear stellar bulge, rather than a spherical excess. Given its non-spherical nature, we argue that the Galactic centre excess is not a dark-matter phenomenon but rather associated with the stellar population of the Galactic bulge and the nuclear bulge.</description><source format="bibcode">2018NatAs...2..387M</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/other/NatAs/2.387</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/IX/67">IX/67 : Incremental Fermi LAT 4th source cat., 4FGL-DR3 (Fermi-LAT 2022)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/J/ApJ/819/44">J/ApJ/819/44 : First Fermi-LAT Inner Galaxy point source cat. 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