Detection of pulsed gamma-rays at energies above 300 GeV from pulsars - T.I.F.R. experiments

Details Detection of pulsed gamma-rays at energies above 300 GeV from pulsars - T.I.F.R. experiments Detection of pulsed gamma-rays at energies above 300 GeV from pulsars - T.I.F.R. experiments

Jun 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981rspta.301..629s&link_type=abstract

(Royal Society, Discussion on Gamma-Ray Astronomy, London, England, Nov. 27, 28, 1980.) Royal Society (London), Philosophical Tr

Astronomy and Astrophysics

Astronomy

2

Energy Spectra, Gamma Ray Astronomy, Gamma Ray Spectra, Pulsars, Stellar Radiation, Gamma Ray Observatory, Radiant Flux Density

Scientific paper

A brief account is given of the search for gamma-rays from pulsars made by the T.I.F.R. group in India. It is concluded that for energies above 300 GeV the flux of pulsed gamma-rays from the Crab and Vela pulsars is much less than would be expected by extrapolation of the spectra measured in the gigaelectronvolt range. It is still not certain whether the pulsars have been detected above 300 GeV because of variability in the apparent signals from year to year.

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