4.6 Article

Planetary transit candidates in the CoRoT LRa01 field

期刊

ASTRONOMY & ASTROPHYSICS
卷 538, 期 -, 页码 -

出版社

EDP SCIENCES S A
DOI: 10.1051/0004-6361/201116968

关键词

techniques: spectroscopic; techniques: photometric; binaries: eclipsing; techniques: radial velocities; planetary systems

资金

  1. Deutsches Zentrum fur Luft- und Raumfahrt (DLR) [50 QM 1004, 50 OW 0204, 50 OW 0603, 50 QP 07011]
  2. Spanish Ministerio de Ciencia e Innovacion [ESP2007-65480-C02-02, AYA2010-20982-C02-02]
  3. W. M. Keck Foundation
  4. SOPHIE spectrograph at the Observatoire de Haute-Provence, France [PNP.08A.MOUT, PNP.09A.MOUT, PNP.10A.MOUT]
  5. FIES spectrograph at the Nordic Optical Telescope [P42-261]
  6. AAOmega multi-object facilities at the Anglo-Australian Telescope
  7. Anglo-Australian Observatory [07B/040, 08B/003]
  8. Alfried Krupp von Bohlen und Halbach Foundation, Essen
  9. [080.D-0151]
  10. [081.C-0388]
  11. [081.C-0413]
  12. [083.C-0186]
  13. [282.C-5015]
  14. Science and Technology Facilities Council [ST/G002266/1] Funding Source: researchfish
  15. UK Space Agency [ST/G002266/2] Funding Source: researchfish
  16. STFC [ST/G002266/1] Funding Source: UKRI

向作者/读者索取更多资源

Context. CoRoT is a pioneering space mission whose primary goals are stellar seismology and extrasolar planets search. Its surveys of large stellar fields generate numerous planetary candidates whose lightcurves have transit-like features. An extensive analytical and observational follow-up effort is undertaken to classify these candidates. Aims. We present the list of planetary transit candidates from the CoRoT LRa01 star field in the Monoceros constellation toward the Galactic anti-center direction. The CoRoT observations of LRa01 lasted from 24 October 2007 to 3 March 2008. Methods. We acquired and analyzed 7470 chromatic and 3938 monochromatic lightcurves. Instrumental noise and stellar variability were treated with several filtering tools by different teams from the CoRoT community. Different transit search algorithms were applied to the lightcurves. Results. Fifty-one stars were classified as planetary transit candidates in LRa01. Thirty-seven (i.e., 73% of all candidates) are good planetary candidates based on photometric analysis only. Thirty-two (i.e., 87% of the good candidates) have been followed-up. At the time of writing twenty-two cases were solved and five planets were discovered: three transiting hot-Jupiters (CoRoT-5b, CoRoT-12b, and CoRoT-21b), the first terrestrial transiting planet (CoRoT-7b), and another planet in the same system (CoRoT-7c, detected by radial velocity survey only). Evidence of another non-transiting planet in the CoRoT-7 system, namely CoRoT-7d, was recently found as well.

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