The DOHA algorithm: A new recipe for cotrending large-scale transiting exoplanet survey light curves

D. Mislis*, S. Pyrzas, K. A. Alsubai, Z. I. Tsvetanov, N. P.E. Vilchez

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

6 Citations (Scopus)

Abstract

We present DOHA, a new algorithm for cotrending photometric light curves obtained by transiting exoplanet surveys. The algorithm employs a novel approach to the traditional 'differential photometry' technique, by selecting the most suitable comparison star for each target light curve, using a two-step correlation search. Extensive tests on real data reveal that DOHA corrects both intra-night variations and long-term systematics affecting the data. Statistical studies conducted on a sample of ~9500 light curves from the Qatar Exoplanet Survey reveal that DOHA-corrected light curves show an rms improvement of a factor of ~2, compared to the raw light curves. In addition, we show that the transit detection probability in our sample can increase considerably, even up to a factor of 7, after applying DOHA.

Original languageEnglish
Pages (from-to)3759-3766
Number of pages8
JournalMonthly Notices of the Royal Astronomical Society
Volume465
Issue number3
DOIs
Publication statusPublished - 1 Mar 2017

Keywords

  • Methods: data analysis
  • Methods: statistical
  • Planets and satellites: detection
  • Techniques: photometric

Fingerprint

Dive into the research topics of 'The DOHA algorithm: A new recipe for cotrending large-scale transiting exoplanet survey light curves'. Together they form a unique fingerprint.

Cite this