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Two Years of Monitoring of Blazars with the OVRO 40 m Telescope at 15 GHz in Support of Fermi-GST

Max-Moerbeck, Walter and Pavlidou, Vasiliki and Pearson, Timothy J. and Readhead, Anthony C. S. and Richards, Joseph and Stevenson, Matthew and Healey, Stephen E. and Romani, Roger W. and Shaw, Michael S. and Zensus, J. A. and Fuhrmann, Lars and Angelakis, Emmanouil and Grainge, Keith and Taylor, Gregory B. (2010) Two Years of Monitoring of Blazars with the OVRO 40 m Telescope at 15 GHz in Support of Fermi-GST. In: Accretion and Ejection in AGNs: A Global View. ASP Conference Series. No.427. Astronomical Society of the Pacific , pp. 199-200. ISBN 978-1-58381-735-3. https://resolver.caltech.edu/CaltechAUTHORS:20110524-100842523

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Abstract

We have continued our monitoring program of ~1200 sources with the Owens Valley Radio Observatory 40 m Telescope. Most of the sources are part of the Candidate Gamma-Ray Blazar Survey (CGRaBS). We have also been observing Targets Of Opportunity triggered by gamma-ray detections and participating in multiwalength campaigns lead by Fermi-GST. Regular program sources are observed twice a week and have been observed for ~24 months at 15 GHz. We use these light curves to study the radio variability and its relation with optical properties. 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. Here we present some example light curves, describe the tools used to study the variability and present some preliminary variability statistics for the sample.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://www.aspbooks.org/a/volumes/article_details/?paper_id=31832PublisherArticle
ORCID:
AuthorORCID
Max-Moerbeck, Walter0000-0002-5491-5244
Pearson, Timothy J.0000-0001-5213-6231
Readhead, Anthony C. S.0000-0001-9152-961X
Romani, Roger W.0000-0001-6711-3286
Angelakis, Emmanouil0000-0001-7327-5441
Taylor, Gregory B.0000-0001-6495-7731
Additional Information:© 2010 Astronomical Society of the Pacific. This work is supported in part by NASA NNX08AW31G and NSF AST-0808050.
Funders:
Funding AgencyGrant Number
NASANNX08AW31G
NSFAST-0808050
Series Name:ASP Conference Series
Issue or Number:427
Record Number:CaltechAUTHORS:20110524-100842523
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20110524-100842523
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:23777
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:24 May 2011 21:42
Last Modified:09 Apr 2020 17:20

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