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Title: A search for UHE cosmic ray from the Crab pulsar/nebula. [PSR 0531+21]

Conference · · AIP Conference Proceedings (American Institute of Physics); (United States)
OSTI ID:5597155
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  1. The University of California, Irvine, California 92717 (USA)
  2. The University of California, Irvine, California 92717 (USA) The University of Maryland, College Park, Maryland 20742-4111 (USA) Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (USA) The University of Notre Dame, Notre Dame, Indiana 46556 (USA) George Mason University, Fairfax, Virginia 22030-4444 (USA) Argonne National Laboratory, Argonne, Illinois 60439-4843 (USA)

A preliminary search is made for continuously pulsed, and burst, emission from the Crab pulsar or its nebula at ultra-high energies using the CYGNUS air shower experiment. No evidence is found for pulsed emission over the entire data set of 1,075 days searched. A 90% confidence upper limit for the flux of cosmic rays at the interpulse phase is 6.9{times}10{sup {minus}14} cm{sup {minus}2}s{sup {minus}1} above 50 TeV. A single day (JD=2447644.5,UTC=66700{ital s} to JD=2447645.5,UTC=11200{ital s}), is found to have a 4.1 {sigma} excess corresponding to a chance probability of 2.2%; no evidence of the pulsar period is found on this day.

OSTI ID:
5597155
Report Number(s):
CONF-9010289-; CODEN: APCPC; TRN: 91-019998
Journal Information:
AIP Conference Proceedings (American Institute of Physics); (United States), Vol. 220:1; Conference: International conference on high energy gamma ray astronomy, Ann Arbor, MI (United States), 2-5 Oct 1990; ISSN 0094-243X
Country of Publication:
United States
Language:
English