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hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorLANDE, J.
dc.contributor.authorACKERMANN, Markus
dc.contributor.authorALLAFORT, A.
hal.structure.identifierAstrophysique Interprétation Modélisation [AIM (UMR7158 / UMR_E_9005 / UM_112)]
dc.contributor.authorBALLET, Jean
dc.contributor.authorBECHTOL, K.
dc.contributor.authorH. BURNETT, T.
hal.structure.identifierLaboratoire Univers et Particules de Montpellier [LUPM]
dc.contributor.authorCOHEN-TANUGI, J.
dc.contributor.authorDRLICA-WAGNER, A.
dc.contributor.authorFUNK, S.
dc.contributor.authorGIORDANO, F.
dc.contributor.authorGRONDIN, M.-H.
dc.contributor.authorKERR, M.
hal.structure.identifierGLAST
dc.contributor.authorLEMOINE-GOUMARD, M.
dc.date.issued2012
dc.identifier.issn0004-637X
dc.description.abstractEnSpatial extension is an important characteristic for correctly associating γ-rayemitting sources with their counterparts at other wavelengths and for obtaining an unbiased model of their spectra. We present a new method for quantifying the spatial extension of sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi ). We perform a series of Monte Carlo simulations to validate this tool and calculate
dc.language.isoen
dc.publisherAmerican Astronomical Society
dc.subject.encatalogs
dc.subject.engamma rays: general
dc.subject.enISM: supernova remnants
dc.subject.enmethods: statistical Online-only material: color figures
dc.title.enSearch for Spatially Extended Fermi 1 -LAT Sources Using Two 2 Years of Data
dc.typeArticle de revue
dc.identifier.doi10.1088/0004-637X/756/1/5
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Phénomènes cosmiques de haute energie [astro-ph.HE]
dc.identifier.arxiv1207.0027
bordeaux.journalThe Astrophysical Journal
bordeaux.page5
bordeaux.volume756
bordeaux.peerReviewedoui
hal.identifierin2p3-00747331
hal.version1
hal.popularnon
hal.audienceNon spécifiée
hal.origin.linkhttps://hal.archives-ouvertes.fr//in2p3-00747331v1
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