Two Years Of Monitoring Of Blazars With The Ovro 40 M Telescope At 15 GHz In Support Of Fermi-GST

Details Two Years Of Monitoring Of Blazars With The Ovro 40 M Telescope At 15 GHz In Support Of Fermi-GST Two Years Of Monitoring Of Blazars With The Ovro 40 M Telescope At 15 GHz In Support Of Fermi-GST

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21441712m&link_type=abstract

American Astronomical Society, AAS Meeting #214, #417.12; Bulletin of the American Astronomical Society, Vol. 41, p.686

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We have monitored 1200 sources with the Owens Valley Radio Observatory 40 m Telescope for 24 months at a frequency of 15GHz. Most of the sources are part of the Candidate Gamma-Ray Blazar Survey (CGRaBS) catalog. We have also been observing "Targets of Opportunity" (ToO) triggered by gamma-ray detections, and participated in multiwavelength campaigns led by the Fermi-GST collaboration. CGRaBS program sources are observed at least twice per week. We use these light curves to study the radio variability and its relationship to the optical properties of these objects. A significant fraction of the bright AGNs detected by Fermi-GST are in our program, which will allow for correlations between the radio and gamma-ray behavior for a number of sources.

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