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Title: KEPLER OBSERVATIONS OF THREE PRE-LAUNCH EXOPLANET CANDIDATES: DISCOVERY OF TWO ECLIPSING BINARIES AND A NEW EXOPLANET

Journal Article · · Astrophysical Journal
 [1]; ;  [2];  [3]; ;  [4];  [5];  [6];  [7]
  1. National Optical Astronomy Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States)
  2. NASA Ames Research Center, Moffett Field, CA 94035 (United States)
  3. National Solar Observatory, 950 North Cherry Avenue, Tucson, AZ 85719 (United States)
  4. NASA Exoplanet Science Institute, California Institute of Technology, 770 South Wilson Avenue Pasadena, CA 91125 (United States)
  5. Department of Physics and Astronomy, Youngstown State University, Youngstown, OH 44555 (United States)
  6. Southern Connecticut State University, New Haven, CT 06515 (United States)
  7. European Southern Observatory, Karl-Schwarzschild-Str 2., 85478 Garching (Germany)

Three transiting exoplanet candidate stars were discovered in a ground-based photometric survey prior to the launch of NASA's Kepler mission. Kepler observations of them were obtained during Quarter 1 of the Kepler mission. All three stars are faint by radial velocity follow-up standards, so we have examined these candidates with regard to eliminating false positives and providing high confidence exoplanet selection. We present a first attempt to exclude false positives for this set of faint stars without high-resolution radial velocity analysis. This method of exoplanet confirmation will form a large part of the Kepler mission follow-up for Jupiter-sized exoplanet candidates orbiting faint stars. Using the Kepler light curves and pixel data, as well as medium-resolution reconnaissance spectroscopy and speckle imaging, we find that two of our candidates are binary stars. One consists of a late-F star with an early M companion, while the other is a K0 star plus a late M-dwarf/brown dwarf in a 19 day elliptical orbit. The third candidate (BOKS-1) is an r = 15 G8V star hosting a newly discovered exoplanet with a radius of 1.12 R{sub Jupiter} in a 3.9 day orbit.

OSTI ID:
21476701
Journal Information:
Astrophysical Journal, Vol. 725, Issue 2; Other Information: DOI: 10.1088/0004-637X/725/2/1633; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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