Study of the Galactic anticentre region at 100 GeV with CELESTE

Details Study of the Galactic anticentre region at 100 GeV with CELESTE Study of the Galactic anticentre region at 100 GeV with CELESTE

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007sf2a.conf..154b&link_type=abstract

SF2A-2007: Proceedings of the Annual meeting of the French Society of Astronomy and Astrophysics held in Grenoble, France, July

Astronomy and Astrophysics

Astrophysics

Scientific paper

Located in the French Pyrénées, CELESTE was the first ground based detector with an energy threshold below 100 GeV. It took data between 1998 and 2004, and allowed flux measurements from the Crab nebula and from the blazars Mrk 421 and Mrk 501. Galactic diffuse gamma-ray emission is the most significant around the Galactic plane, [-5,+5] degrees of Galactic latitude. From the large samples on the Crab Nebula, we have selected Crab OFF data with different Galactic latitudes, in order to analyse the diffuse emission. After criteria applied on sky position, atmospheric conditions and detector stability, we obtain 108 min of data in the Galactic anticentre region, providing a new limit on the diffuse emission with ACT detectors.

Affiliated with

Also associated with

No associations

Rating

Study of the Galactic anticentre region at 100 GeV with CELESTE 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 Study of the Galactic anticentre region at 100 GeV with CELESTE, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Study of the Galactic anticentre region at 100 GeV with CELESTE will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-789728