Planetary transit candidates in COROT-IRa01 field
arXiv:0907.5150 · doi:10.1051/0004-6361/200911882
Abstract
Context: CoRoT is a pioneering space mission devoted to the analysis of stellar variability and the photometric detection of extrasolar planets. Aims: We present the list of planetary transit candidates detected in the first field observed by CoRoT, IRa01, the initial run toward the Galactic anticenter, which lasted for 60 days. Methods: We analysed 3898 sources in the coloured bands and 5974 in the monochromatic band. Instrumental noise and stellar variability were taken into account using detrending tools before applying various transit search algorithms. Results: Fifty sources were classified as planetary transit candidates and the most reliable 40 detections were declared targets for follow-up ground-based observations. Two of these targets have so far been confirmed as planets, COROT-1b and COROT-4b, for which a complete characterization and specific studies were performed.
11 pages, 8 figures
References in corpus (8)
- Transiting exoplanets from the CoRoT space mission VIII. CoRoT-7b: the first Super-Earth with measured radius
- The effect of red noise on planetary transit detection
- Transiting exoplanets from the CoRoT space mission I - CoRoT-Exo-1b: a low-density short-period planet around a G0V star
- Transiting exoplanets from the CoRoT space mission IV: CoRoT-Exo-4b: A transiting planet in a 9.2 day synchronous orbit
- Noise properties of the CoRoT data: a planet-finding perspective
- Characterization of CoRoT target fields with BEST: Identification of periodic variable stars in the IR01 field
- The BAST algorithm for transit detection
- Detecting transits from Earth-sized planets around Sun-like stars
Cited by in corpus (4)
- Ground-based photometry of space-based transit detections: Photometric follow-up of the CoRoT mission
- Rate and nature of false positives in the CoRoT exoplanet search
- Planetary transit candidates in the CoRoT LRa01 field
- Wavelet-based filter methods to detect small transiting planets in stellar light curves