Contribution of point sources to the soft gamma-ray Galactic emission

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dc.creatorTerrier, Regis
dc.creatorLebrun, Francois
dc.creatorBelanger, Guillaume
dc.creatorGoldwurm, Andrea
dc.creatorStrong, Andrew W.
dc.creatorSchoenfelder, Volker
dc.creatorBouchet, Laurent
dc.creatorRoques, Jean-Pierre
dc.creatorParmar, Arvind
dc.date2004-05-11
dc.date.accessioned2026-07-07T06:30:30Z
dc.date.available2026-07-07T06:30:30Z
dc.descriptionThe nature of the soft gamma-ray (20-200 keV) Galactic emission has been a matter of debate for a long time. Previous experiments have tried to separate the point source contribution from the real interstellar emission, but with a rather poor spatial resolution, they concluded that the interstellar emission could be a large fraction of the total Galactic emission. INTEGRAL, having both high resolution and high sensitivity, is well suited to reassess more precisely this problem. Using the INTEGRAL core program Galactic Center Deep Exposure (GCDE), we estimate the contribution of detected point sources to the total Galactic flux.
dc.descriptionProceedings of the 5th INTEGRAL Workshop, Munich 16-20 February 2004. ESA SP-552
dc.identifierhttps://arxiv.org/abs/astro-ph/0405207
dc.identifierhttp://arxiv.org/abs/astro-ph/0405207
dc.identifierProceedings of the 5th INTEGRAL Workshop on The INTEGRAL Universe (2004) 513-518
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/98358
dc.subjectAstrophysics
dc.titleContribution of point sources to the soft gamma-ray Galactic emission
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