Spectral and timing analysis of The γ-ray Pulsar PSR J0007+7303 in the supernova remnant CTA1

Details Spectral and timing analysis of The γ-ray Pulsar PSR J0007+7303 in the supernova remnant CTA1 Spectral and timing analysis of The γ-ray Pulsar PSR J0007+7303 in the supernova remnant CTA1

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1357..294g&link_type=abstract

RADIO PULSARS: AN ASTROPHYSICAL KEY TO UNLOCK THE SECRETS OF THE UNIVERSE. AIP Conference Proceedings, Volume 1357, pp. 294-296

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, Magnetic Fields, Gamma-Ray Production, Wind, Supernova Remnants, Electric And Magnetic Fields, Gamma-Ray Sources, Gamma-Ray Bursts, Galactic Winds And Fountains

Scientific paper

Pulsar PSR J0007+7303 in supernova remnant CTA1 was the first γ-ray pulsar to be discovered with Fermi Large Area Telescope using a blind-search technique [3]. The inferred surface magnetic field (1.1×1013 G) is among the highest detected from the 65 γ-ray pulsars already detected with the Fermi LAT. Detailed studies of the spectral emission and variability studies of this source are presented.

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