Understanding limitations in the determination of the diffuse Galactic gamma-ray emission

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dc.creatorMoskalenko, I. V.
dc.creatorDigel, S. W.
dc.creatorPorter, T. A.
dc.creatorReimer, O.
dc.creatorStrong, A. W.
dc.date2006-09-28
dc.date.accessioned2026-07-07T11:04:13Z
dc.date.available2026-07-07T11:04:13Z
dc.descriptionWe discuss uncertainties and possible sources of errors associated with the determination of the diffuse Galactic gamma-ray emission using the EGRET data. Most of the issues will be relevant also in the GLAST era. The focus here is on issues that impact evaluation of dark matter annihilation signals against the diffuse gamma-ray emission of the Milky Way.
dc.description4 pages, to appear in proceedings of 7th UCLA symposium on Sources and Detection of Dark Matter and Dark Energy in the Universe (Marina del Rey, Feb 22-24, 2006); Nuclear Physics B, in press
dc.identifierhttps://arxiv.org/abs/astro-ph/0609768
dc.identifierhttp://arxiv.org/abs/astro-ph/0609768
dc.identifierNucl.Phys.Proc.Suppl.173:44-47,2007
dc.identifierdoi:10.1016/j.nuclphysbps.2007.08.022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/188816
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleUnderstanding limitations in the determination of the diffuse Galactic gamma-ray emission
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