STACEE Observations of Active Galactic Nuclei

Details STACEE Observations of Active Galactic Nuclei STACEE Observations of Active Galactic Nuclei

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.0742m&link_type=abstract

American Astronomical Society, HEAD meeting #9, #7.42; Bulletin of the American Astronomical Society, Vol. 38, p.356

Astronomy and Astrophysics

Astrophysics

Scientific paper

The Solar Tower Atmospheric Cherenkov Effect Experiment (STACEE) is a ground-based experiment that is sensitive to gamma rays above 100 GeV. STACEE's extragalactic observing program has included both high-frequency peaked as well as low-frequency peaked BL Lac objects (HBLs & LBLs). STACEE's sensitivity to astrophysical sources at an energy range 100 - 500 GeV allows it to explore LBLs, with their synchrotron peaks at lower energies. The sources observed include the HBLs: Markarian 421, Markarian 501,1H 1426+428 and 1ES 1218+304, and the LBLs: 3C 66A, OJ 287 and W Comae. Both the 3C 66A and Mrk 421 observations were part of intensive multiwavelength campaigns. We present a summary of these observations.

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