A Search for Point Sources of Cosmic Primary Rays Which Produce Single Muon Tracks at Ground Level

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dc.creatorRoesch, A.
dc.creatorCarpenter, J.
dc.creatorDesch, S.
dc.creatorGress, J.
dc.creatorLin, T. F.
dc.creatorPoirier, J.
dc.date2000-08-25
dc.date.accessioned2026-07-07T01:55:07Z
dc.date.available2026-07-07T01:55:07Z
dc.descriptionAn increased data sample of identified secondary muons is collected at detection level. Project GRAND identifies secondary cosmic ray muons from electrons utilizing a thin steel absorber and tracking (PWC) chambers. The resulting angular resolution for the primary is about +/- 5 degrees. Since there is a 1.5% probability that a 100 GeV gamma primary will produce a single muon track at ground level, the high statistics allows a search for angular enhancements due to gammas. More than 100 billion muons are identified and analyzed. A table of stellar sources is examined.
dc.description4 pgs; includes 1 fig. and 2 tables. HE.3.2.10 in 26th ICRC, 2, 104, (1999)
dc.identifierhttps://arxiv.org/abs/astro-ph/0008405
dc.identifierhttp://arxiv.org/abs/astro-ph/0008405
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1545
dc.subjectAstrophysics
dc.titleA Search for Point Sources of Cosmic Primary Rays Which Produce Single Muon Tracks at Ground Level
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