AGN Monitoring with the Whipple 10m Gamma-ray Telescope

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

May 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...20910909h&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #109.09; Bulletin of the American Astronomical Society,

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Since September 2005, the Whipple 10m Gamma-ray Telescope has been operated primarily as an AGN monitor. The five Northern Hemisphere blazars which have already been detected at Whipple, Markarian 421, H1426+428, Markarian 501, 1ES 1959+650 and 1ES 2344+514, are monitored routinely each night that they are visible. To encourage and co-ordinate observations of these AGN at other wavelengths, a web page containing the observing timetable and the preliminary light curves at TeV wavelengths is maintained and is publicly accessible:
http://veritas.sao.arizona.edu/content/blogsection/6/40/
Thanks to the efforts of a large number of collaborators, a significant amount of data over the entire spectrum have been gathered on these five AGN. We report here on the current status of this AGN multiwavelength, monitoring campaign which is ongoing, and present light curves of radio, optical, infra-red, x-ray and gamma-ray data.

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