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The UMC extensive air shower array: Results and prospects
dc.contributor.authorMatthews, J.en_US
dc.date.accessioned2011-11-15T16:04:28Z
dc.date.available2011-11-15T16:04:28Z
dc.date.issued1990-03-20en_US
dc.identifier.citationMatthews, J. (1990). "The UMC extensive air shower array: Results and prospects." AIP Conference Proceedings 203(1): 210-213. <http://hdl.handle.net/2027.42/87597>en_US
dc.identifier.otherAPCPCS-203-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87597
dc.description.abstractThe Utah‐Michigan‐Chicago array addresses the need for greater measurement sensitivity in searches for ultra‐high energy gamma rays. Results from the Utah‐Michigan experiment demonstrate the power of muon rejection. Even if photons interact in unconventional ways, the combination of CASA and the large muon array will measure these effects.en_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleThe UMC extensive air shower array: Results and prospectsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Physics, University of Michigan, Ann Arbor, Michigan, USA 48109en_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87597/2/210_1.pdf
dc.identifier.doi10.1063/1.39153en_US
dc.identifier.sourceParticle astrophysicsen_US
dc.owningcollnamePhysics, Department of


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