Observation of the VELA gamma-ray pulsar with the GAMMA-1 telescope

Details Observation of the VELA gamma-ray pulsar with the GAMMA-1 telescope Observation of the VELA gamma-ray pulsar with the GAMMA-1 telescope

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...97..325o&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 97, no. 1, p. 325-327.

Astronomy and Astrophysics

Astronomy

1

Gamma Ray Astronomy, Gamma Ray Telescopes, Pulsars, Emission Spectra, Light Curve, Stellar Spectra

Scientific paper

Observations of PSR0933 with the GAMMA-1 telescope in the summer of 1990 and spring of 1991 are presented. The mean 300-5000 MeV flux of the whole pulsed emission is found to be consistent with the time-averaged COS-B result. The 30-300 MeV flux suggests that the pulsar was observed in a low intensity state. The emission from the first peak appears softer than the second peak. The variation of the spectra over time is investigated.

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