Aims. We present a catalog of point γ-ray sources detected by the EGRET detector on the Compton Gamma Ray Observatory. We used the entire γ-ray dataset of reprocessed photons at energies above 100 MeV and new Galactic interstellar emission models based on CO, HI, dark gas, and interstellar radiation field data. Two different assumptions are used to describe the cosmic-ray distribution in the Galaxy to analyse the systematic uncertainties in source detection and characterization.
No takes yet. Share an insight, caveat, or question.
Casandjian et al. (2008) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: