The Lick AGN Monitoring Project 2. Photometric Light Curves

Details The Lick AGN Monitoring Project 2. Photometric Light Curves The Lick AGN Monitoring Project 2. Photometric Light Curves

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21330603w&link_type=abstract

American Astronomical Society, AAS Meeting #213, #306.03; Bulletin of the American Astronomical Society, Vol. 41, p.276

Astronomy and Astrophysics

Astronomy

Scientific paper

The Lick AGN Monitoring Project (LAMP) targeted 13 nearby Seyfert 1 galaxies with the intent of measuring the masses of their central black holes using reverberation mapping. In conjunction with the spectroscopic monitoring, we obtained broad-band B and V imaging observations on most nights between the months of February and May 2008. The sample of 13 objects was divided between four telescopes: the 30-inch Katzman Automatic Imaging Telescope (KAIT), the 2-meter Multicolor Active Galactic Nuclei Monitoring (MAGNUM) telescope, the Palomar 60-inch telescope, and the 32-inch Tenagra II telescope. In this talk, we will discuss the observational methods, the photometric measurements, the resultant light curves, and the variability characteristics of each object.

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