Very high energy gamma rays from the Crab Nebula

Details Very high energy gamma rays from the Crab Nebula Very high energy gamma rays from the Crab Nebula

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..139t&link_type=abstract

In NASA. Goddard Space Fligh Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 139-142 (SEE N85-33902 22-93)

Physics

Cerenkov Counters, Crab Nebula, Flux Density, Gamma Rays, Light Curve, Pulsars, Cygnus Constellation, Energy Spectra, Galactic Radiation, Light Curve, Point Sources, Protons, Pulses

Scientific paper

Observations of the Crab pulsar using the atmospheric Cerenkov technique were conducted for 22 hours on Sept. - Oct. 1984. The light curve obtained shows a single peak at approximately the position of the expected main peak with a significant level of 3.2 σ. The pulsed flux above 200 GeV is 2.5±0.8×10-11cm-2s-1.

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