Status and current sensitivity of the CELESTE experiment

Details Status and current sensitivity of the CELESTE experiment Status and current sensitivity of the CELESTE experiment

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..558..540c&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: International Symposium. AIP Conference Proceedings, Volume 558, pp. 540-543 (2001).

Astronomy and Astrophysics

Astronomy

Gamma-Ray Astronomy, Astronomical Instruments, Gamma-Ray Sources (Astronomical), Supernova Remnants, Gamma-Ray Detection, Gamma-Ray Spectra, Astronomical Spectra

Scientific paper

The CELESTE experiment uses the heliostats of an old solar farm in the French Pyrenees to detect gamma ray air showers by the atmospheric Cerenkov technique. CELESTE has been operating since November 1999 with an array of 40 heliostats fully instrumented with 1 GHz flash ADCs. Significant advances have been made in the detector simulations and in the data analysis techniques. We report here on results from recent observations of the Crab nebula above an energy threshold of 50 GeV. The results and simulations illustrate the current sensitivity of the experiment. .

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