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    The Sloan Digital Sky Survey Reverberation Mapping Project: PhotometricgandiLight Curves

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    Kinemuchi_2020_ApJS_250_10.pdf
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    Final Published Version
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    Author
    Kinemuchi, K.
    Hall, Patrick B.
    McGreer, Ian
    Kochanek, C. S. cc
    Grier, Catherine J.
    Trump, Jonathan
    Shen, Yue
    Brandt, W. N. cc
    Wood-Vasey, W. M. cc
    Fan, Xiaohui
    Peterson, Bradley M.
    Schneider, Donald P.
    Hernandez Santisteban, Juan V.
    Horne, Keith
    Chen, Yuguang
    Eftekharzadeh, Sarah
    Guo, Yucheng
    Jia, Siyao
    Li, Feng
    Li, Zefeng
    Nie, Jundan
    Ponder, Kara A.
    Rogerson, Jesse cc
    Zhang, Tianmen
    Zou, Hu cc
    Jiang, Linhua
    Ho, Luis C.
    Kneib, Jean-Paul
    Petitjean, Patrick
    Palanque-Delabrouille, Nathalie
    Yeche, Christophe
    Show allShow less
    Affiliation
    Univ Arizona, Steward Observ
    Issue Date
    2020-09
    Keywords
    Active galactic nuclei
    
    Metadata
    Show full item record
    Publisher
    IOP PUBLISHING LTD
    Citation
    Kinemuchi, K., Hall, P. B., McGreer, I., Kochanek, C. S., Grier, C. J., Trump, J., ... & Yeche, C. (2020). The Sloan Digital Sky Survey Reverberation Mapping Project: Photometric g and i Light Curves. The Astrophysical Journal Supplement Series, 250(1), 10.
    Journal
    ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
    Rights
    © 2020 The American Astronomical Society. All rights reserved.
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    The Sloan Digital Sky Survey (SDSS) Reverberation Mapping program monitors 849 active galactic nuclei (AGNs) both spectroscopically and photometrically. The photometric observations used in this work span over 4 yr and provide an excellent baseline for variability studies of these objects. We present the photometric light curves from 2014 to 2017 obtained by the Steward Observatory's Bok telescope and the Canada-France-Hawaii telescope with MegaCam. We provide details on the data acquisition and processing of the data from each telescope, the difference imaging photometry used to produce the light curves, and the calculation of a variability index to quantify each AGN's variability. We find that the Welch-Stetson J index provides a useful characterization of AGN variability and can be used to select AGNs for further study.
    Note
    Immediate access
    ISSN
    0067-0049
    EISSN
    1538-4365
    DOI
    10.3847/1538-4365/aba43f
    Version
    Final published version
    ae974a485f413a2113503eed53cd6c53
    10.3847/1538-4365/aba43f
    Scopus Count
    Collections
    UA Faculty Publications

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