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arXiv:0711.4278 (astro-ph)
[Submitted on 27 Nov 2007]

Title:Gamma-Ray Pulsar Studies with GLAST

Authors:D. J. Thompson
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Abstract: Some pulsars have their maximum observable energy output in the gamma-ray band, offering the possibility of using these high-energy photons as probes of the particle acceleration and interaction processes in pulsar magnetospheres. After an extended hiatus between satellite missions, the recently-launched AGILE mission and the upcoming Gamma-ray Large Area Space Telescope (GLAST) Large Area Telescope (LAT) will allow gamma-ray tests of the theoretical models developed based on past discoveries. With its greatly improved sensitivity, better angular resolution, and larger energy reach than older instruments, GLAST LAT should detect dozens to hundreds of new gamma-ray pulsars and measure luminosities, light curves, and phase-resolved spectra with unprecedented resolution. It will also have the potential to find radio-quiet pulsars like Geminga, using blind search techniques. Cooperation with radio and X-ray pulsar astronomers is an important aspect of the LAT team's planning for pulsar studies.
Comments: 8 pages, 5 figures. To appear in the proceedings of "40 Years of Pulsars: Millisecond Pulsars, Magnetars, and More", August 12-17, 2007, McGill University, Montreal, Canada
Subjects: Astrophysics (astro-ph)
Cite as: arXiv:0711.4278 [astro-ph]
  (or arXiv:0711.4278v1 [astro-ph] for this version)
  https://doi.org/10.48550/arXiv.0711.4278
Journal reference: AIP Conf.Proc.983:56-63,2008
Related DOI: https://doi.org/10.1063/1.2900301

Submission history

From: David J. Thompson [view email]
[v1] Tue, 27 Nov 2007 15:16:08 UTC (548 KB)
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