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Published October 2011 | Published
Journal Article Open

Terms Photometry of Known Transiting Exoplanets

Abstract

The Transit Ephemeris Refinement and Monitoring Survey conducts radial velocity and photometric monitoring of known exoplanets in order to refine planetary orbits and predictions of possible transit times. This effort is primarily directed toward planets not known to transit, but a small sample of our targets consists of known transiting systems. Here we present precision photometry for six WASP (Wide Angle Search for Planets) planets acquired during their transit windows. We perform a Markov Chain Monte Carlo analysis for each planet and combine these data with previous measurements to redetermine the period and ephemerides for these planets. These observations provide recent mid-transit times which are useful for scheduling future observations. Our results improve the ephemerides of WASP-4b, WASP-5b, and WASP-6b and reduce the uncertainties on the mid-transit time for WASP-29b. We also confirm the orbital, stellar, and planetary parameters of all six systems.

Additional Information

© 2011 American Astronomical Society. Received 2011 May 3; accepted 2011 July 29; published 2011 September 8. The authors thank Andrés Jordán for providing support for the observations at CTIO, and the anonymous referee who provided helpful comments that improved the manuscript. We also thank C. Hellier for the ESO NTT/EFOSC light curve of WASP-19. D.D. is supported by an FQRNT scholarship and an IPAC Visiting Graduate fellowship. M.R. acknowledges support from ALMA-CONICYT projects 31090015 and 31080021. The Center for Exoplanets and Habitable Worlds is supported by the Pennsylvania State University, the Eberly College of Science, and the Pennsylvania Space Grant Consortium.

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Created:
August 22, 2023
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October 24, 2023