The transit light curve project. VIII. Six occultations of the exoplanet tres-3

Joshua N. Winn, Matthew J. Holman, Avi Shporer, José Fernndez, Tsevi Mazeh, David W. Latham, David Charbonneau, Mark E. Everett

Research output: Contribution to journalArticlepeer-review

19 Scopus citations

Abstract

We present photometry of the exoplanet host star TrES-3 spanning six occultations (secondary eclipses) of its giant planet. No flux decrements were detected, leading to 99%-confidence upper limits on the planet-to-star flux ratio of 2.4 × 10-4, 5.0 × 10-4, and 8.6 × 10-4 in the i-, z-, and R-bands respectively. The corresponding upper limits on the planet's geometric albedo are 0.30, 0.62, and 1.07. The upper limit in the i-band rules out the presence of highly reflective clouds, and is only a factor of 2-3 above the predicted level of thermal radiation from the planet.

Original languageEnglish
Pages (from-to)267-271
Number of pages5
JournalAstronomical Journal
Volume136
Issue number1
DOIs
StatePublished - 1 Jul 2008

Keywords

  • Planetary systems
  • Stars: individual (TrES-3, GSC 0308900929)
  • Techniques: photometric

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