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- W2488956632 abstract "We have developed a method for quantifying the flux variabilities of high energy gamma ray sources. We have applied this method to 128 sources listed in the second catalog of sources detected with the Energetic Gamma Ray Experiment Telescope (EGRET) (Thompson et. al. 1995). These sources include the Large Magellanic Cloud, 5 pulsars, 41 active galactic nuclei (AGN), and 81 sources not yet identified with known objects. Our data include photon maps (E > 100 MeV) from 134 EGRET viewing periods spanning a roughly 3 year period. Each source was observed in 3-20 viewing periods ranging from a few days to 3 weeks in length. For each observation, a source flux was calculated using the method of maximum likelihood (Mattox et al . 1996) which simultaneously estimates the strength of the Galactic and isotropic diffuse emission, and that of a point source distributed as the EGRET point spread function." @default.
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- W2488956632 date "1996-01-01" @default.
- W2488956632 modified "2023-09-23" @default.
- W2488956632 title "Variability of CGRO/EGRET Gamma Ray Sources" @default.
- W2488956632 cites W3012165734 @default.
- W2488956632 doi "https://doi.org/10.1017/s0252921100041889" @default.
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