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Granite, a new very high energy gamma-ray telescope

dc.contributor.authorAkerlof, Carl W.en_US
dc.contributor.authorCawley, M. F.en_US
dc.contributor.authorFegan, D. J.en_US
dc.contributor.authorHillas, A. M.en_US
dc.contributor.authorLamb, R. C.en_US
dc.contributor.authorLewis, D. A.en_US
dc.contributor.authorMeyer, D. I.en_US
dc.contributor.authorWeekes, T. C.en_US
dc.date.accessioned2006-04-10T13:49:31Z
dc.date.available2006-04-10T13:49:31Z
dc.date.issued1990-03en_US
dc.identifier.citationAkerlof, C. W., Cawley, M. F., Fegan, D. J., Hillas, A. M., Lamb, R. C., Lewis, D. A., Meyer, D. I., Weekes, T. C. (1990/03)."Granite, a new very high energy gamma-ray telescope." Nuclear Physics B - Proceedings Supplements 14(1): 237-243. <http://hdl.handle.net/2027.42/28708>en_US
dc.identifier.urihttp://www.sciencedirect.com/science/article/B6TVD-473MC6V-2R/2/1c7e7b16e75e64c6a12c12e066120ff7en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/28708
dc.description.abstractA international collaboration of astrophysicists plan to construct a new 10-meter diameter gamma-ray Cerenkov telescope at the Whipple Observatory on Mt. Hopkins in Arizona. By operatin in coincidence with the original 10-meter reflector, the sensitivity for gamma-ray detection will improve by more than an order of magnitude. The new telescope, named GRANITE (for amma-ay strophysics ew maging lescope), will include a 109-element imaging photon detector wit a 0.2[deg] pixel size. The entire system consists of a steerable alt-azimuth mount, a faceted mirror assembly, a highly segmented photon detector, and ancillary data acquisition and control electronics. This telescope is considered an engineering prototype for a large array of Cherenkov detectors which will further enhance our ability to detect astrophysical sources of very high energy gamma rays.en_US
dc.format.extent681367 bytes
dc.format.extent3118 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherElsevieren_US
dc.titleGranite, a new very high energy gamma-ray telescopeen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbsecondlevelNuclear Engineering and Radiological Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumRandall Laboratory of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAen_US
dc.contributor.affiliationumRandall Laboratory of Physics, University of Michigan, Ann Arbor, Michigan 48109, USAen_US
dc.contributor.affiliationotherPhysics Department, St. Patrick's College, Maynooth, Co., Kildare, Irelanden_US
dc.contributor.affiliationotherPhysics Department, University College, Dublin, 4., Irelanden_US
dc.contributor.affiliationotherPhysics Department, University of Leeds, Leeds, United Kingdomen_US
dc.contributor.affiliationotherPhysics Department, Iowa State University, Ames, Iowa. 50011, USAen_US
dc.contributor.affiliationotherPhysics Department, Iowa State University, Ames, Iowa. 50011, USAen_US
dc.contributor.affiliationotherFred Lawrence Whipple Observatory, Harvard-Smithsonian Center for Astrophysics, P.O.Box 97, Amado, Arizona 85645, USAen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/28708/1/0000528.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1016/0920-5632(90)90427-Ven_US
dc.identifier.sourceNuclear Physics B - Proceedings Supplementsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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