Using Gaussian processes to model light curves in the presence of flickering: the eclipsing cataclysmic variable ASASSN-14ag

McAllister, M.J., Littlefair, S.P., Dhillon, V.S. et al. (10 more authors) (2016) Using Gaussian processes to model light curves in the presence of flickering: the eclipsing cataclysmic variable ASASSN-14ag. Monthly Notices of the Royal Astronomical Society. ISSN 0035-8711

Abstract

Metadata

Authors/Creators:
  • McAllister, M.J.
  • Littlefair, S.P.
  • Dhillon, V.S.
  • Marsh, T.R.
  • Ashley, R.P.
  • Bours, M.C.P.
  • Breedt, E.
  • Hardy, L.K.
  • Hermes, J.J.
  • Kengkriangkrai, S.
  • Kerry, P.
  • Rattanasoon, S.
  • Sahman, D.I.
Copyright, Publisher and Additional Information: © 2016 Oxford University Press. This is an author produced version of a paper subsequently published in Monthly Notices of the Royal Astronomical Society. Uploaded in accordance with the publisher's self-archiving policy.
Keywords: binaries; close binaries; eclipsing stars; dwarf novae stars; individual; ASASSN-14ag stars; cataclysmic variables methods; data analysis techniques; Gaussian processes
Dates:
  • Published: 26 September 2016
  • Published (online): 26 September 2016
Institution: The University of Sheffield
Academic Units: The University of Sheffield > Faculty of Science (Sheffield) > Department of Physics and Astronomy (Sheffield)
Depositing User: Symplectic Sheffield
Date Deposited: 03 Oct 2016 14:51
Last Modified: 21 Mar 2018 21:01
Published Version: http://dx.doi.org/10.1093/mnras/stw2417
Status: Published
Publisher: Oxford University Press
Refereed: Yes
Identification Number: https://doi.org/10.1093/mnras/stw2417
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