Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2011-10-31
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
2011 Fermi Symposium proceedings - eConf C110509
Scientific paper
AGILE pointed observations performed from July 9, 2007 to October 30, 2009 cover a very large time interval, with a \gamma-ray dataset useful to perform studies of medium to high brightness galactic sources in the 30 MeV -- 50 GeV energy range. We present a study of the 1AGL galactic sources in the E > 100 MeV band, over the complete Agile pointed Observation Blocks (OBs) archive. The first AGILE Gamma-Ray Imaging Detector (GRID) catalog included a sample of 47 sources (1AGL; Pittori et al. 2009), detected with a conservative analysis over the first year of operations dataset. In the analysis here reported we used data obtained with an improved full Field of View (FOV) event filter, on a much larger (about 27.5 months) observation dataset, analyzing the merging of all data and each OB separately. The data processing resulted in an improved source list as compared to the 1AGL one, particularly in complex regions of the galactic plane. We present here some results on the revised 1AGL galactic sources and on the variability of some of them.
Bulgarelli Andrea
Chen Andrew W.
for the AGILE Collaboration
Giommi Paolo
Lucarelli Fabrizio
No associations
LandOfFree
A variability study of the AGILE first catalog of γ-ray sources on 2.3 years of AGILE pointed observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A variability study of the AGILE first catalog of γ-ray sources on 2.3 years of AGILE pointed observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A variability study of the AGILE first catalog of γ-ray sources on 2.3 years of AGILE pointed observations will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-466272