Variations in the Very-High-Energy Gamma-Ray Radiation from the Blazar H 1426+428

Details Variations in the Very-High-Energy Gamma-Ray Radiation from the Blazar H 1426+428 Variations in the Very-High-Energy Gamma-Ray Radiation from the Blazar H 1426+428

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005arep...49..859f&link_type=abstract

Astronomy Reports, vol. 49, Issue 11, p.859-862

Astronomy and Astrophysics

Astronomy

1

Scientific paper

Observations of the blazar H 1426+428 were carried with on the GT-48 Cerenkov telescope of the Crimean Astrophysical Observatory from April 15 to April 25, 2004. Analysis of the observational data shows an excess of very-high-energy photons (≥1 TeV) in the direction of the source, with a statistical confidence of 5.8 σ. A flash lasting no more than seven days was detected.

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