Detection of 10-100 MeV γ-Rays from the Crab Nebula Pulsar NP 0532

Details Detection of 10-100 MeV γ-Rays from the Crab Nebula Pulsar NP 0532 Detection of 10-100 MeV γ-Rays from the Crab Nebula Pulsar NP 0532

Nov 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972natur.240..221a&link_type=abstract

Nature, Volume 240, Issue 5378, pp. 221-224 (1972).

Physics

30

Scientific paper

Pulsed γ-ray emission from NP 0532 has been detected up to 100
MeV. For the main pulse from 10 to 30 MeV the signal to noise is
(5-6σ). The energy spectrum of the main pulse from 1 keV to 100
MeV can be fitted by a single power law of index (-0.9).

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