TY - JOUR
T1 - The Sloan Digital Sky Survey Reverberation Mapping Project
T2 - Photometric g and i Light Curves
AU - Kinemuchi, K.
AU - Hall, Patrick B.
AU - McGreer, Ian
AU - Kochanek, C. S.
AU - Grier, Catherine J.
AU - Trump, Jonathan
AU - Shen, Yue
AU - Brandt, W. N.
AU - Wood-Vasey, W. M.
AU - Fan, Xiaohui
AU - Peterson, Bradley M.
AU - Schneider, Donald P.
AU - Hernández Santisteban, Juan V.
AU - Horne, Keith
AU - Chen, Yuguang
AU - Eftekharzadeh, Sarah
AU - Guo, Yucheng
AU - Jia, Siyao
AU - Li, Feng
AU - Li, Zefeng
AU - Nie, Jundan
AU - Ponder, Kara A.
AU - Rogerson, Jesse
AU - Zhang, Tianmen
AU - Zou, Hu
AU - Jiang, Linhua
AU - Ho, Luis C.
AU - Kneib, Jean Paul
AU - Petitjean, Patrick
AU - Palanque-Delabrouille, Nathalie
AU - Yeche, Christophe
N1 - Publisher Copyright:
© 2020. The American Astronomical Society. All rights reserved..
PY - 2020/9
Y1 - 2020/9
N2 - 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.
AB - 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.
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U2 - 10.3847/1538-4365/aba43f
DO - 10.3847/1538-4365/aba43f
M3 - Review article
AN - SCOPUS:85091387711
SN - 0067-0049
VL - 250
JO - Astrophysical Journal, Supplement Series
JF - Astrophysical Journal, Supplement Series
IS - 1
M1 - 10
ER -