Constraints on the steady and pulsed very high energy gamma-ray emission from observations of PSR B1951+32/CTB 80 with the MAGIC Telescope

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dc.creatorMAGIC Collaboration
dc.creatorAlbert, J.
dc.date2007-02-02
dc.date2007-12-10
dc.date.accessioned2026-07-07T11:42:45Z
dc.date.available2026-07-07T11:42:45Z
dc.descriptionWe report on very high energy gamma-observations with the MAGIC Telescope of the pulsar PSR B1951+32 and its associated nebula, CTB 80. Our data constrain the cutoff energy of the pulsar to be less than 32 GeV, assuming the pulsed gamma-ray emission to be exponentially cut off. The upper limit on the flux of pulsed gamma-ray emission above 75 GeV is 4.3*10^-11 photons cm^-2 sec^-1, and the upper limit on the flux of steady emission above 140 GeV is 1.5*10^-11 photons cm^-2 sec^-1. We discuss our results in the framework of recent model predictions and other studies.
dc.description7 pages, 7 figures, replaced with published version
dc.identifierhttps://arxiv.org/abs/astro-ph/0702077
dc.identifierhttp://arxiv.org/abs/astro-ph/0702077
dc.identifierAstrophys.J.669:1143-1149,2007
dc.identifierdoi:10.1086/521807
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/200995
dc.subjectAstrophysics
dc.titleConstraints on the steady and pulsed very high energy gamma-ray emission from observations of PSR B1951+32/CTB 80 with the MAGIC Telescope
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