Blazar Monitoring with the Whipple 10 m Gamma-ray Telescope

Details Blazar Monitoring with the Whipple 10 m Gamma-ray Telescope Blazar Monitoring with the Whipple 10 m Gamma-ray Telescope

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008head...10.4101k&link_type=abstract

American Astronomical Society, HEAD meeting #10, #41.01

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Scientific paper

Since September 2005, the Whipple 10 m Gamma-ray Telescope has been used primarily to monitor known TeV AGN. The five Northern Hemisphere blazars that have been previously detected at Whipple, Markarian 421, H1426+428, Markarian 501, 1ES 1959+650 and 1ES 2344+514, are monitored each night that they are visible.
To encourage and co-ordinate observations of these AGN at other wavelengths, the observing timetable and preliminary light curves for the TeV observations are provided on a publicly accessible website: veritas.sao.arizona.edu/content/blogsection/6/40
A number of multiwavelength observing campaigns have been undertaken by numerous collaborators in conjunction with the Whipple program and a significant amount of data has been accumulated. We report here on the status of these multiwavelength observations and present light curves of radio, optical, X-ray and gamma-ray data.

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