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Prospects for Pulsar Studies with the GLAST Large Area TelescopeThe Large Area Telescope (LAT) on the Gamma-ray Large Area Space Telescope (GLAST), due to launch in November 2007, will have unprecedented sensitivity and energy resolution for gamma-rays in the range of 30 MeV to 200 GeV. GLAST is therefore expected to provide major advances in the understanding of high-energy emission from rotation-powered p ulsars. As the only presently known galactic GeV source class, pulsar s will be one of the most important sources for study with GLAST. The main science goals of the LAT for pulsar studies include an increase in the number of detected radio-loud and radio-quiet gamma-ray pulsar s, including millisecond pulsars, giving much better statistics for e lucidating population characteristics, measurement of the high-energy spectrum and the shape of spectral cutoffs and determining pulse profiles for a variety of pulsars of different age. Further, measurement of phase-resolved spectra and energy dependent pulse profiles of the brighter pulsars should allow detailed tests of magnetospheric partic le acceleration and radiation mechanisms, by comparing data with theo retical models that have been developed. Additionally, the LAT will have the sensitivity to allow blind pulsation searches of nearly all un identified EGRET sources, to possibly uncover more radio-quiet Geming a-like pulsars.
Document ID
20070030045
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Harding, Alice K.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 23, 2013
Publication Date
March 29, 2007
Subject Category
Astronomy
Meeting Information
Meeting: Pulsar Searching and Thai-ming- 207-SKA
Location: Krabi
Country: Thailand
Start Date: March 29, 2007
End Date: April 5, 2007
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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