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The Lick AGN Monitoring Project 2011: Photometric Light Curves

Author(s): Pancoast, Anna; Skielboe, Andreas; Pei, Liuyi; Bennert, Vardha N; Sand, David J; et al

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dc.contributor.authorPancoast, Anna-
dc.contributor.authorSkielboe, Andreas-
dc.contributor.authorPei, Liuyi-
dc.contributor.authorBennert, Vardha N-
dc.contributor.authorSand, David J-
dc.contributor.authorBarth, Aaron J-
dc.contributor.authorJoner, Michael D-
dc.contributor.authorThorman, Shawn-
dc.contributor.authorSchmidt, Thomas-
dc.contributor.authorTreu, Tommaso-
dc.contributor.authorBrewer, Brendon J-
dc.contributor.authorLi, Weidong-
dc.contributor.authorBuehler, Tabitha-
dc.contributor.authorLaney, C David-
dc.contributor.authorCanalizo, Gabriela-
dc.contributor.authorFilippenko, Alexei V-
dc.contributor.authorGreene, Jenny E.-
dc.contributor.authorMalkan, Matthew A-
dc.contributor.authorStern, Daniel-
dc.contributor.authorWoo, Jong-Hak-
dc.date.accessioned2019-08-29T17:04:06Z-
dc.date.available2019-08-29T17:04:06Z-
dc.date.issued2019-01-20en_US
dc.identifier.citationPancoast, Anna, Skielboe, Andreas, Pei, Liuyi, Bennert, Vardha N, Sand, David J, Barth, Aaron J, Joner, Michael D, Thorman, Shawn, Schmidt, Thomas, Treu, Tommaso, Brewer, Brendon J, Li, Weidong, Buehler, Tabitha, Laney, C David, Canalizo, Gabriela, Filippenko, Alexei V, Greene, Jenny E, Malkan, Matthew A, Stern, Daniel, Woo, Jong-Hak. (2019). The Lick AGN Monitoring Project 2011: Photometric Light Curves. ASTROPHYSICAL JOURNAL, 871 (10.3847/1538-4357/aaf806en_US
dc.identifier.issn0004-637X-
dc.identifier.urihttp://arks.princeton.edu/ark:/88435/pr11q8b-
dc.description.abstractIn Spring 2011, the Lick AGN Monitoring Project observed a sample of 15 bright, nearby Seyfert 1 galaxies in the V-band as part of a reverberation mapping campaign. The observations were taken at six ground-based telescopes, including the West Mountain Observatory 0.91 m telescope, the 0.76 m Katzman Automatic Imaging Telescope, 0.6 m Super-LOTIS at Kitt Peak, the Palomar 60 inch telescope, and the 2 m Faulkes telescopes North and South. The V-band light curves measure the continuum variability of our sample of Seyferts on an almost daily cadence for 2-3 months. We use image-subtraction software to isolate the variability of the Seyfert nucleus from the constant V-band flux of the host galaxy for the most promising targets, and we adopt standard aperture photometry techniques for the targets with smaller levels of variability. These V-band light curves will be used, with measurements of the broad emission line flux, to measure supermassive black hole masses and to constrain the geometry and dynamics of the broad-line region through dynamical modeling techniques.en_US
dc.language.isoen_USen_US
dc.relationhttp://simbad.u-strasbg.fr/simbad/sim-ref?querymethod=bib&simbo=on&submit=submit+bibcode&bibcode=2019ApJ...871..108Pen_US
dc.relation.ispartofASTROPHYSICAL JOURNALen_US
dc.rightsFinal published version. Article is made available in OAR by the publisher's permission or policy.en_US
dc.titleThe Lick AGN Monitoring Project 2011: Photometric Light Curvesen_US
dc.typeJournal Articleen_US
dc.identifier.doidoi:10.3847/1538-4357/aaf806-
dc.date.eissued2019-01-25en_US
dc.identifier.eissn1538-4357-
pu.type.symplectichttp://www.symplectic.co.uk/publications/atom-terms/1.0/journal-articleen_US

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