Jonelle L. Walsh et al. 2009 ApJS 185 156 doi:10.1088/0067-0049/185/1/156
Jonelle L. Walsh1, Takeo Minezaki2, Misty C. Bentz1,15, Aaron J. Barth1, Nairn Baliber3,4, Weidong Li5, Daniel Stern6, Vardha Nicola Bennert3, Timothy M. Brown4, Gabriela Canalizo7,8, Alexei V. Filippenko5, Elinor L. Gates9, Jenny E. Greene10,15, Matthew A. Malkan11, Yu Sakata2,12, Rachel A. Street3,4, Tommaso Treu3,16, Jong-Hak Woo11,14,15 and Yuzuru Yoshii2,13
Show affiliationsThe Lick AGN Monitoring Project targeted 13 nearby Seyfert 1 galaxies with the intent of measuring the masses of their central black holes using reverberation mapping. The sample includes 12 galaxies selected to have black holes with masses roughly in the range 106-107 M ☉, as well as the well-studied active galactic nucleus (AGN) NGC 5548. In conjunction with a spectroscopic monitoring campaign, we obtained broadband B and V images on most nights from 2008 February through 2008 May. The imaging observations were carried out by four telescopes: the 0.76 m Katzman Automatic Imaging Telescope, the 2 m Multicolor Active Galactic Nuclei Monitoring telescope, the Palomar 60 inch (1.5 m) telescope, and the 0.80 m Tenagra II telescope. Having well-sampled light curves over the course of a few months is useful for obtaining the broad-line reverberation lag and black hole mass, and also allows us to examine the characteristics of the continuum variability. In this paper, we discuss the observational methods and the photometric measurements, and present the AGN continuum light curves. We measure various variability characteristics of each of the light curves. We do not detect any evidence for a time lag between the B- and V-band variations, and we do not find significant color variations for the AGNs in our sample.
Issue 1 (2009 November)
Received 2009 June 24, accepted for publication 2009 September 25
Published 2009 October 22
Jonelle L. Walsh et al. 2009 ApJS 185 156
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