Observations of the Pulsar PSR B1951+32 with the Solar Tower Atmospheric Cherenkov Effect Experiment

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dc.creatorKildea, J.
dc.creatorZweerink, J.
dc.creatorBall, J.
dc.creatorCarson, J. E.
dc.creatorCovault, C. E.
dc.creatorDriscoll, D. D.
dc.creatorFortin, P.
dc.creatorGingrich, D. M.
dc.creatorHanna, D. S.
dc.creatorJarvis, A.
dc.creatorLindner, T.
dc.creatorMueller, C.
dc.creatorMukherjee, R.
dc.creatorOng, R. A.
dc.creatorRagan, K.
dc.creatorWilliams, D. A.
dc.date2007-10-25
dc.date.accessioned2026-07-07T08:38:34Z
dc.date.available2026-07-07T08:38:34Z
dc.descriptionWe present the analysis and results of 12.5 hours of high-energy gamma-ray observations of the EGRET-detected pulsar PSR B1951+32 using the Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE). STACEE is an atmospheric Cherenkov detector, in Albuquerque, New Mexico, that detects cosmic gamma rays using the shower-front-sampling technique. STACEE's sensitivity to astrophysical sources at energies around 100 GeV allows it to investigate emission from gamma-ray pulsars with expected pulsed emission cutoffs below 100 GeV. We discuss the observations and analysis of STACEE's PSR 1951+32 data, accumulated during the 2005 and 2006 observing seasons.
dc.description4 pages, 1 figure, ICRC 2007 conference proceedings
dc.identifierhttps://arxiv.org/abs/0710.4623
dc.identifierhttp://arxiv.org/abs/0710.4623
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/140773
dc.subjectAstrophysics
dc.titleObservations of the Pulsar PSR B1951+32 with the Solar Tower Atmospheric Cherenkov Effect Experiment
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