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Title: GROUND-BASED MULTISITE OBSERVATIONS OF TWO TRANSITS OF HD 80606b

Journal Article · · Astrophysical Journal
 [1];  [2];  [3];  [4]; ; ; ;  [5];  [6]; ;  [7];  [8];  [9]; ;  [10];  [11]; ;  [12]; ;  [13]
  1. Las Cumbres Observatory Global Telescope Network, 6740 Cortona Drive, Suite 102, Santa Barbara, CA 93117 (United States)
  2. Department of Physics and Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA 02139 (United States)
  3. Georg-August-Universitaet, Institut fuer Astrophysik, Friedrich-Hund-Platz 1, 37077 Goettingen (Germany)
  4. Department of Astronomy, University of Florida, 211 Bryant Space Science Center, Gainesville, FL 32611-2055 (United States)
  5. Department of Physics and Astronomy, University of Pittsburgh, 3941 O'Hara Street, Pittsburgh, PA 15260 (United States)
  6. Department of Physics and Astronomy, Pomona College, 610 North College Avenue, Claremont, CA 91711 (United States)
  7. Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139 (United States)
  8. Laboratoire d'Astrophysique de Marseille, Universite de Provence, CNRS (UMR 6110), 38 rue Frederic Joliot Curie, 13388 Marseille Cedex 13 (France)
  9. Department of Astronomy, San Diego State University, 5500 Campanile Drive, San Diego, CA 92182 (United States)
  10. Astrophysics Research Centre, School of Mathematics and Physics, Queens University, University Road, Belfast, BT7 1NN (United Kingdom)
  11. DeKalb Observatory H63, Auburn, IN 46706 (United States)
  12. Institut d'Astrophysique de Paris, UMR7095 CNRS, Universite Pierre and Marie Curie, 98 bis boulevard Arago, 75014 Paris (France)
  13. Instituto de Astrofisica de Canarias, C. Via Lactea S/N, 38205 La Laguna, Tenerife (Spain)

We present ground-based optical observations of the 2009 September and 2010 January transits of HD 80606b. Based on three partial light curves of the 2009 September event, we derive a midtransit time of T{sub c} [HJD] = 2455099.196 {+-} 0.026, which is about 1{sigma} away from the previously predicted time. We observed the 2010 January event from nine different locations, with most phases of the transit being observed by at least three different teams. We determine a midtransit time of T{sub c} [HJD] = 2455210.6502 {+-} 0.0064, which is within 1.3{sigma} of the time derived from a Spitzer observation of the same event.

OSTI ID:
21464672
Journal Information:
Astrophysical Journal, Vol. 722, Issue 1; Other Information: DOI: 10.1088/0004-637X/722/1/880; ISSN 0004-637X
Country of Publication:
United States
Language:
English

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