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dc.contributor.authorLeane, Rebecca K
dc.contributor.authorSlatyer, Tracy R
dc.date.accessioned2021-10-27T20:36:05Z
dc.date.available2021-10-27T20:36:05Z
dc.date.issued2019
dc.identifier.urihttps://hdl.handle.net/1721.1/136577
dc.description.abstract© 2019 American Physical Society. Statistical evidence has previously suggested that the galactic center GeV excess (GCE) originates largely from point sources, and not from annihilating dark matter. We examine the impact of unmodeled source populations on identifying the true origin of the GCE using non-Poissonian template fitting (NPTF) methods. In a proof-of-principle example with simulated data, we discover that unmodeled sources in the Fermi bubbles can lead to a dark matter signal being misattributed to point sources by the NPTF. We discover striking behavior consistent with a mismodeling effect in the real Fermi data, finding that large artificial injected dark matter signals are completely misattributed to point sources. Consequently, we conclude that dark matter may provide a dominant contribution to the GCE after all.
dc.language.isoen
dc.publisherAmerican Physical Society (APS)
dc.relation.isversionof10.1103/PHYSREVLETT.123.241101
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.
dc.sourceAPS
dc.titleRevival of the Dark Matter Hypothesis for the Galactic Center Gamma-Ray Excess
dc.typeArticle
dc.relation.journalPhysical Review Letters
dc.eprint.versionFinal published version
dc.type.urihttp://purl.org/eprint/type/JournalArticle
eprint.statushttp://purl.org/eprint/status/PeerReviewed
dc.date.updated2021-07-01T11:49:32Z
dspace.orderedauthorsLeane, RK; Slatyer, TR
dspace.date.submission2021-07-01T11:49:33Z
mit.journal.volume123
mit.journal.issue24
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Needed


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