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arXiv · astro-ph/0312590

Blazar Flaring Rates Measured with GLAST

C. D. Dermer·B. L. Dingus
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Abstract

We derive the minimum observing time scales to detect a blazar at a given flux level with the LAT on GLAST in the scanning and pointing modes. Based upon Phase 1 observations with EGRET, we predict the GLAST detection rate of blazar flares at different flux levels. With some uncertainty given the poor statistics of bright blazars, we predict that a blazar flare with integral flux >~ 200e-8 ph(> 100 MeV) cm^{-2} s^{-1}, which are the best candidates for Target of Opportunity pointings and extensive temporal and spectral studies, should occur every few days.

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C. D. Dermer, B. L. Dingus. 2003-12-22. Blazar Flaring Rates Measured with GLAST. https://doi.org/10.1016/j.newar.2003.12.013

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