Angular power spectrum of the diffuse gamma-ray emission as measured by the Fermi Large Area Telescope and constraints on its dark matter interpretation

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dc.contributor.authorFornasa, M.
dc.contributor.authorCuoco, A.
dc.contributor.authorZavala, J.
dc.contributor.authorGaskins, J.
dc.contributor.authorSánchez Conde, M.
dc.contributor.authorGómez Vargas, Germán Arturo
dc.contributor.authorKomatsu, E.
dc.contributor.authorLinden, T.
dc.contributor.authorPrada, F.
dc.contributor.authorZandanel, F.
dc.contributor.authorMorselli, A.
dc.date.accessioned2021-05-13T17:49:38Z
dc.date.available2021-05-13T17:49:38Z
dc.date.issued2016
dc.fuente.origenConveris
dc.identifier.doi10.1103/PhysRevD.94.123005
dc.identifier.eissn2470-0029
dc.identifier.issn2470-0010
dc.identifier.urihttps://doi.org/10.1103/PhysRevD.94.123005
dc.identifier.urihttps://repositorio.uc.cl/handle/11534/57980
dc.issue.numeroNo. 12
dc.language.isoen
dc.nota.accesoContenido completo
dc.revistaPhysical Review Des_ES
dc.rightsacceso abierto
dc.titleAngular power spectrum of the diffuse gamma-ray emission as measured by the Fermi Large Area Telescope and constraints on its dark matter interpretationes_ES
dc.typeartículo
dc.volumenVol. 94
sipa.codpersvinculados1013833
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