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The GALEX Time Domain Survey. II. Wavelength-Dependent Variability of Active Galactic Nuclei in the Pan-STARRS1 Medium Deep Survey

Hung, T. and Gezari, S. and Jones, D. O. and Kirshner, R. P. and Chornock, R. and Berger, E. and Rest, A. and Huber, M. and Narayan, G. and Scolnic, D. and Waters, C. and Wainscoat, R. and Martin, D. C. and Forster, K. and Neill, J. D. (2016) The GALEX Time Domain Survey. II. Wavelength-Dependent Variability of Active Galactic Nuclei in the Pan-STARRS1 Medium Deep Survey. Astrophysical Journal, 833 (2). Art. No. 226. ISSN 0004-637X. http://resolver.caltech.edu/CaltechAUTHORS:20161220-093154418

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Abstract

We analyze the wavelength-dependent variability of a sample of spectroscopically confirmed active galactic nuclei selected from near-UV (NUV) variable sources in the GALEX Time Domain Survey that have a large amplitude of optical variability (difference-flux S/N > 3) in the Pan-STARRS1 Medium Deep Survey (PS1 MDS). By matching GALEX and PS1 epochs in five bands (NUV, g_(P1), r_(P1), i_(P1), z_(P1)) in time, and taking their flux difference, we create co-temporal difference-flux spectral energy distributions (ΔƒSEDs) using two chosen epochs for each of the 23 objects in our sample, on timescales of about a year. We confirm the "bluer-when-brighter" trend reported in previous studies, and measure a median spectral index of the ΔƒSEDs of ɑ_⋋ = 2.1 that is consistent with an accretion disk spectrum. We further fit the ΔƒSEDs of each source with a standard accretion disk model in which the accretion rate changes from one epoch to the other. In our sample, 17 out of 23 (~74%) sources are described well by this variable accretion-rate disk model, with a median average characteristic disk temperature T^* of 1.2 x 10^5 K that is consistent with the temperatures expected, given the distribution of accretion rates and black hole masses inferred for the sample. Our analysis also shows that the variable accretion rate model is a better fit to the ΔƒSEDs than a simple power law.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.3847/1538-4357/833/2/226DOIArticle
http://iopscience.iop.org/article/10.3847/1538-4357/833/2/226PublisherArticle
https://arxiv.org/abs/1609.06307arXivDiscussion Paper
ORCID:
AuthorORCID
Berger, E.0000-0002-9392-9681
Wainscoat, R.0000-0002-1341-0952
Neill, J. D.0000-0002-0466-1119
Additional Information:© 2016 American Astronomical Society. Received 2016 June 27. Accepted 2016 September 20. Published 2016 December 19. We thank the anonymous referee for valuable comments and suggestions that helped to improve this paper. S.G. was supported in part by NSF CAREER grant 1454816. Some of the observations reported here were obtained at the MMT Observatory, a joint facility of the Smithsonian Institution and the University of Arizona. We thank R. Foley for his contribution to the PS1 transients program. The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under Grant No. AST-1238877, and the University of Maryland.
Group:Space Astrophysics Laboratory
Funders:
Funding AgencyGrant Number
NSFAST-1454816
Institute for AstronomyUNSPECIFIED
University of HawaiiUNSPECIFIED
Pan-STARRS Project OfficeUNSPECIFIED
Max-Planck SocietyUNSPECIFIED
Max Planck Institute for Astronomy (MPIA)UNSPECIFIED
Max Planck Institute for Extraterrestrial PhysicsUNSPECIFIED
Johns Hopkins UniversityUNSPECIFIED
Durham UniversityUNSPECIFIED
University of EdinburghUNSPECIFIED
Queen's University BelfastUNSPECIFIED
Harvard-Smithsonian Center for AstrophysicsUNSPECIFIED
Las Cumbres Observatory Global Telescope Network IncorporatedUNSPECIFIED
National Central University of TaiwanUNSPECIFIED
NASANNX08AR22G
NSFAST-1238877
University of Maryland UNSPECIFIED
Subject Keywords:accretion, accretion disks; black hole physics; galaxies: nuclei; surveys; ultraviolet: general
Record Number:CaltechAUTHORS:20161220-093154418
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20161220-093154418
Official Citation:T. Hung et al 2016 ApJ 833 226
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:72968
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:20 Dec 2016 18:56
Last Modified:22 Mar 2019 00:57

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