Y.-F. Jiang
Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves
Jiang, Y.-F.; Green, P.J.; Greene, J.E.; Morganson, E.; Shen, Y.; Pancoast, A.; MacLeod, C.L.; Anderson, S.F.; Brandt, W.N.; Grier, C.J.; Rix, H.-W.; Ruan, J.J.; Protopapas, P.; Scott, C.; Burgett, W.S.; Hodapp, K.W.; Huber, M.E.; Kaiser, N.; Kudritzki, R.P.; Magnier, E.A.; Metcalfe, N.; Tonry, J.T.; Wainscoat, R.J.; Waters, C.
Authors
P.J. Green
J.E. Greene
E. Morganson
Y. Shen
A. Pancoast
C.L. MacLeod
S.F. Anderson
W.N. Brandt
C.J. Grier
H.-W. Rix
J.J. Ruan
P. Protopapas
C. Scott
W.S. Burgett
K.W. Hodapp
M.E. Huber
N. Kaiser
R.P. Kudritzki
E.A. Magnier
Dr Nigel Metcalfe nigel.metcalfe@durham.ac.uk
Assistant Professor
J.T. Tonry
R.J. Wainscoat
C. Waters
Abstract
As photons from different bands emerge from different radial ranges in the accretion disk, the lags constrain the sizes of the accretion disks. We select 240 quasars with redshifts of z ≈ 1 or z ≈ 0.3 that are relatively emission-line free. The light curves are sampled from day to month timescales, which makes it possible to detect lags on the scale of the light crossing time of the accretion disks. With the code JAVELIN, we detect typical lags of several days in the rest frame between the g band and the riz bands. The detected lags are ~2–3 times larger than the light crossing time estimated from the standard thin disk model, consistent with the recently measured lag in NGC 5548 and microlensing measurements of quasars. The lags in our sample are found to increase with increasing luminosity. Furthermore, the increase in lags going from g − r to g − i and then to g − z is slower than predicted in the thin disk model, particularly for high-luminosity quasars. The radial temperature profile in the disk must be different from what is assumed. We also find evidence that the lags decrease with increasing line ratios between ultraviolet Fe ii lines and Mg ii, which may point to changes in the accretion disk structure at higher metallicity.
Citation
Jiang, Y., Green, P., Greene, J., Morganson, E., Shen, Y., Pancoast, A., …Waters, C. (2017). Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves. Astrophysical Journal, 836(2), Article 186. https://doi.org/10.3847/1538-4357/aa5b91
Journal Article Type | Article |
---|---|
Acceptance Date | Jan 13, 2017 |
Online Publication Date | Feb 21, 2017 |
Publication Date | Feb 21, 2017 |
Deposit Date | Mar 30, 2017 |
Publicly Available Date | Mar 31, 2017 |
Journal | Astrophysical Journal |
Print ISSN | 0004-637X |
Electronic ISSN | 1538-4357 |
Publisher | American Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 836 |
Issue | 2 |
Article Number | 186 |
DOI | https://doi.org/10.3847/1538-4357/aa5b91 |
Public URL | https://durham-repository.worktribe.com/output/1361133 |
Files
Published Journal Article
(2.1 Mb)
PDF
Copyright Statement
© 2017. The American Astronomical Society. All rights reserved.
You might also like
The VST ATLAS quasar survey I: Catalogue of photometrically selected quasar candidates
(2023)
Journal Article
VST ATLAS galaxy cluster catalogue I: cluster detection and mass calibration
(2023)
Journal Article
The local hole: a galaxy underdensity covering 90 per cent of sky to ≈200 Mpc
(2022)
Journal Article
The nature of sub-millimetre galaxies II: an ALMA comparison of SMG dust heating mechanisms
(2022)
Journal Article
Downloadable Citations
About Durham Research Online (DRO)
Administrator e-mail: dro.admin@durham.ac.uk
This application uses the following open-source libraries:
SheetJS Community Edition
Apache License Version 2.0 (http://www.apache.org/licenses/)
PDF.js
Apache License Version 2.0 (http://www.apache.org/licenses/)
Font Awesome
SIL OFL 1.1 (http://scripts.sil.org/OFL)
MIT License (http://opensource.org/licenses/mit-license.html)
CC BY 3.0 ( http://creativecommons.org/licenses/by/3.0/)
Powered by Worktribe © 2025
Advanced Search