Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-11-17
Astron.Astrophys.337:25-30,1998
Astronomy and Astrophysics
Astrophysics
6 pages including 2 figures
Scientific paper
Observational and theoretical results indicate that low-redshift BL Lacertae objects are the most likely extragalactic sources to be detectable at TeV energies. In this paper we present the results of observations of 4 BL Lacertae objects (PKS0521-365, EXO0423.4-0840, PKS2005-489 and PKS2316-423) made between 1993 and 1996 with the CANGAROO 3.8m imaging Cherenkov telescope. During the period of these observations the gamma-ray energy threshold of the 3.8m telescope was ~2TeV. Searches for steady long-term emission have been made, and, inspired by the TeV flares detected from Mkn421 and Mkn501, a search on a night-by-night timescale has also been performed for each source. Comprehensive Monte Carlo simulations are used to estimate upper limits for both steady and short timescale emission.
Dazeley S. A.
Edwards Philip G.
Hara Tabito
Hayami Yuichi
Holder Jamie
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