Physics
Scientific paper
Feb 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011nimpa.630...22v&link_type=abstract
Nuclear Instruments and Methods in Physics Research Section A, Volume 630, Issue 1, p. 22-27.
Physics
Scientific paper
The full coverage extensive air shower detector ARGO-YBJ, located in Tibet at 4300 m of altitude, has monitored the sky at gamma ray energy E>0.6TeV in the declination band from -10° to +70°. In 424 days the Crab Nebula and Mrk421 have been detected with a significance, respectively, of 7.0 and 8.0 standard deviations. The analysis of the cosmic ray background in the same sky band, has revealed the existence of a significant excess of the cosmic ray flux in two localized regions of angular size 10°-30°, confirming previous indications. The origin of such excesses is still unexplained. Concerning the gamma ray sources, the measured spectrum of the Crab Nebula is dN/dE=(3.7±0.8)×10-11E-2.67photonscm-2s-1TeV-1, in agreement with other experiments. During 2008 the observed Mrk421 flux was highly variable, with the strongest flares in March-June, in good correlation with X-ray data. One of the most intense flares occurred in the first half of June and has been deeply studied by different detectors in the energy range from optical to 100 MeV gamma rays, but only partially up to TeV energies, since the moonlight hampered the Cherenkov telescope measurements during the second and most intense part of the emission. Our data complete these observations, with the detection of a signal of intensity of about 7 Crab units on June 11-13, with a statistical significance of 4.2 standard deviations. The observed flux is consistent with a prediction made in the framework of the Synchrotron Self-Compton model, in which the flare is caused by a rapid acceleration of leptons in the jet.
ARGO-YBJ Collaboration
Vernetto Silvia
No associations
LandOfFree
Results from the ARGO-YBJ experiment 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 Results from the ARGO-YBJ experiment, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Results from the ARGO-YBJ experiment will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1133533