The Lick AGN Monitoring Project 2011: Photometric Light Curves
Astrophysical Journal, ISSN: 1538-4357, Vol: 871, Issue: 1, Page: 1-10
2019
- 6Citations
- 133Usage
- 10Captures
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Metrics Details
- Citations6
- Citation Indexes6
- CrossRef6
- Usage133
- Downloads129
- Abstract Views4
- Captures10
- Readers10
- 10
Article Description
In 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.
Bibliographic Details
http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=85062043591&origin=inward; http://dx.doi.org/10.3847/1538-4357/aaf806; https://iopscience.iop.org/article/10.3847/1538-4357/aaf806; https://digitalcommons.calpoly.edu/phy_fac/584; https://digitalcommons.calpoly.edu/cgi/viewcontent.cgi?article=1583&context=phy_fac; https://dx.doi.org/10.3847/1538-4357/aaf806; https://validate.perfdrive.com/9730847aceed30627ebd520e46ee70b2/?ssa=ade80d3f-db08-45fb-b843-da9c1a00d9f9&ssb=93851285148&ssc=https%3A%2F%2Fiopscience.iop.org%2Farticle%2F10.3847%2F1538-4357%2Faaf806&ssi=b02a88de-cnvj-4046-94c4-06f633eed63a&ssk=botmanager_support@radware.com&ssm=45869813947062562898007072611227608&ssn=22fd6194339ed19af64406e3578ef807acc26402f074-4cb6-43cc-ba908e&sso=23d3e5d5-86644739f8a5117897b4e5832af9c5502408186462d2651c&ssp=17093003571728663016172913202736261&ssq=03415024841959597653275883518015207985818&ssr=MzQuMjM2LjI2LjMx&sst=com.plumanalytics&ssu=&ssv=&ssw=&ssx=eyJyZCI6ImlvcC5vcmciLCJfX3V6bWYiOiI3ZjYwMDAwMTkwYjQzMC04NzFlLTRjOGEtODhjNS1hOTI5ZGQ5NTBhYzkxNzI4Njc1ODgzNDM1NDcyNTM1OTAyLTQ0OGQ3MWUzNTAxYTEyMjQ4OTc5NCIsInV6bXgiOiI3ZjkwMDA1MjAyNTk2Ny04NzMxLTQ5ZGUtODY0OC1jY2U1NWI5ZTRiYWM3LTE3Mjg2NzU4ODM0MzY0NzI1MzU5MDEtNTRlNTBkNWM1MWE0NjliOTg5NzkxIn0=
American Astronomical Society
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