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dc.contributor.authorLeane, Rebecca K
dc.contributor.authorSlatyer, Tracy R
dc.date.accessioned2021-10-27T20:23:44Z
dc.date.available2021-10-27T20:23:44Z
dc.date.issued2020
dc.identifier.urihttps://hdl.handle.net/1721.1/135500
dc.description.abstractWe reexamine evidence that the Galactic Center Excess (GCE) originates primarily from point sources (PSs). We show that in our region of interest, non-Poissonian template fitting evidence for GCE PSs is an artifact of unmodeled north-south asymmetry of the GCE. This asymmetry is strongly favored by the fit (although it is unclear if this is physical), and when it is allowed, the preference for PSs becomes insignificant. We reproduce this behavior in simulations, including detailed properties of the spurious PS population. We conclude that the non-Poissonian template fitting evidence for GCE PSs is highly susceptible to certain systematic errors and should not at present be taken to robustly disfavor a dominantly smooth GCE.
dc.language.isoen
dc.publisherAmerican Physical Society (APS)
dc.relation.isversionof10.1103/PHYSREVLETT.125.121105
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.titleSpurious Point Source Signals in the Galactic Center 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.updated2021-07-09T15:48:28Z
dspace.orderedauthorsLeane, RK; Slatyer, TR
dspace.date.submission2021-07-09T15:48:29Z
mit.journal.volume125
mit.journal.issue12
mit.licensePUBLISHER_POLICY
mit.metadata.statusAuthority Work and Publication Information Needed


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