Variable classification in the LSST era: exploring a model for quasi-periodic light curves. Issue 2 (9th March 2017)
- Record Type:
- Journal Article
- Title:
- Variable classification in the LSST era: exploring a model for quasi-periodic light curves. Issue 2 (9th March 2017)
- Main Title:
- Variable classification in the LSST era: exploring a model for quasi-periodic light curves
- Authors:
- Zinn, J. C.
Kochanek, C. S.
Kozłowski, S.
Udalski, A.
Szymański, M. K.
Soszyński, I.
Wyrzykowski, Ł.
Ulaczyk, K.
Poleski, R.
Pietrukowicz, P.
Skowron, J.
Mróz, P.
Pawlak, M. - Abstract:
- Abstract: The Large Synoptic Survey Telescope (LSST) is expected to yield ∼10 7 light curves over the course of its mission, which will require a concerted effort in automated classification. Stochastic processes provide one means of quantitatively describing variability with the potential advantage over simple light-curve statistics that the parameters may be physically meaningful. Here, we survey a large sample of periodic, quasi-periodic and stochastic Optical Gravitational Lensing Experiment-III variables using the damped random walk (DRW; CARMA(1, 0)) and quasi-periodic oscillation (QPO; CARMA(2, 1)) stochastic process models. The QPO model is described by an amplitude, a period and a coherence time-scale, while the DRW has only an amplitude and a time-scale. We find that the periodic and quasi-periodic stellar variables are generally better described by a QPO than a DRW, while quasars are better described by the DRW model. There are ambiguities in interpreting the QPO coherence time due to non-sinusoidal light-curve shapes, signal-to-noise ratio, error mischaracterizations and cadence. Higher order implementations of the QPO model that better capture light-curve shapes are necessary for the coherence time to have its implied physical meaning. Independent of physical meaning, the extra parameter of the QPO model successfully distinguishes most of the classes of periodic and quasi-periodic variables we consider.
- Is Part Of:
- Monthly notices of the Royal Astronomical Society. Volume 468:Issue 2(2017)
- Journal:
- Monthly notices of the Royal Astronomical Society
- Issue:
- Volume 468:Issue 2(2017)
- Issue Display:
- Volume 468, Issue 2 (2017)
- Year:
- 2017
- Volume:
- 468
- Issue:
- 2
- Issue Sort Value:
- 2017-0468-0002-0000
- Page Start:
- 2189
- Page End:
- 2205
- Publication Date:
- 2017-03-09
- Subjects:
- methods: data analysis -- stars: oscillations -- stars: variables: Cepheids -- stars: variables: general -- stars: variables: RR Lyrae -- Magellanic Clouds
Astronomy -- Periodicals
Periodicals
520.5 - Journal URLs:
- http://mnras.oxfordjournals.org/ ↗
http://onlinelibrary.wiley.com/journal/10.1111/(ISSN)1365-2966 ↗
http://www.blackwell-synergy.com/issuelist.asp?journal=mnr ↗
http://www.blackwell-synergy.com/loi/mnr ↗
http://ukcatalogue.oup.com/ ↗ - DOI:
- 10.1093/mnras/stx586 ↗
- Languages:
- English
- ISSNs:
- 0035-8711
- Deposit Type:
- Legaldeposit
- View Content:
- Available online (eLD content is only available in our Reading Rooms) ↗
- Physical Locations:
- British Library DSC - 5943.000000
British Library DSC - BLDSS-3PM
British Library HMNTS - ELD Digital store - Ingest File:
- 24992.xml