Results from Milagrito on TeV emission by active Galactic nuclei

Details Results from Milagrito on TeV emission by active Galactic nuclei Results from Milagrito on TeV emission by active Galactic nuclei

Jun 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..515..144m&link_type=abstract

GeV-TeV GAMMA RAY ASTROPHYSICS WORKSHOP: Towards a Major Atmospheric Cherenkov Detector VI. AIP Conference Proceedings, Volume

Astronomy and Astrophysics

Astronomy

Gamma-Ray Astronomy, Gamma-Ray Sources (Astronomical), Bl Lac-Type Objects, Cosmic Background Radiation, Cosmic Ray Showers, Emission, Astronomical Instruments, Gamma-Ray Detection

Scientific paper

Milagrito was a preliminary phase of the Milagro experiment and operated from February 1997 to May 1998. Milagrito was a water-Cherenkov detector for air showers produced by gamma rays (and background cosmic rays). The data have been studied for emission from several nearby blazars. Emission from Markarian 501 is detected coincident with the large flare observed in 1997 by several atmospheric Cherenkov telescopes. .

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