The first planet detected in the WTS: an inflated hot Jupiter in a 3.35 d orbit around a late F star

Cappetta, M.; Saglia, R. P.; Birkby, J. L.; Koppenhoefer, J.; Pinfield, D. J.; Hodgkin, S. T.; Cruz, P.; Kovács, G.; Sipőcz, B.; Barrado, D; Nefs, B; Pavlenko, Y. V.; Fossati, L.; del Burgo, C.; Martin, E. L.; Snellen, I.; Barnes, J.; Bayo, A.; Campbell, D. A.; Catalan, S.; Galvez-Ortiz, M. C.; Goulding, N.; Haswell, C.; Ivanyuk, O.; Jones, H. R.; Kuznetsov, M.; Lodieu, N.; Marocco, F.; Mislis, D.; Murgas, F.; Napiwotzki, R.; Palle, E.; Pollacco, D.; Sarro Baro, L.; Solano, E.; Steele, P.; Stoev, H.; Tata, R. and Zendejas, J. (2012). The first planet detected in the WTS: an inflated hot Jupiter in a 3.35 d orbit around a late F star. Monthly Notices of the Royal Astronomical Society, 427(3) pp. 1877–1890.

DOI: https://doi.org/10.1111/j.1365-2966.2012.21937.x

URL: http://mnras.oxfordjournals.org/content/427/3/1877

Abstract

We report the discovery of WTS-1b, the first extrasolar planet found by the WFCAM Transit Survey, which began observations at the 3.8-m United Kingdom Infrared Telescope (UKIRT) in 2007 August. Light curves comprising almost 1200 epochs with a photometric precision of better than 1 per cent to J ˜ 16 were constructed for ˜60 000 stars and searched for periodic transit signals. For one of the most promising transiting candidates, high-resolution spectra taken at the Hobby-Eberly Telescope (HET) allowed us to estimate the spectroscopic parameters of the host star, a late-F main-sequence dwarf (V = 16.13) with possibly slightly subsolar metallicity, and to measure its radial velocity variations. The combined analysis of the light curves and spectroscopic data resulted in an orbital period of the substellar companion of 3.35 d, a planetary mass of 4.01 ± 0.35 M_J and a planetary radius of 1.49_-0.18^+0.16 R_J. WTS-1b has one of the largest radius anomalies among the known hot Jupiters in the mass range 3-5 M_J. The high irradiation from the host star ranks the planet in the pM class.

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About

• Item ORO ID
• 36565
• Item Type
• Journal Item
• ISSN
• 1365-2966
• Project Funding Details

• Funded Project Name	Project ID	Funding Body
  Not Set	Not Set	European Commission
  Not Set	Not Set	STFC (Science & Technology Facilities Council)
  Not Set	Not Set	MICINN
  Not Set	Not Set	Fundação para a Ciência e a Tecnologia (FCT)-Portugal

• Keywords
• photometric techniques; radial velocities; detection of planets and satellites; planets and satellites; planetary systems
• Academic Unit or School
• Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
  Faculty of Science, Technology, Engineering and Mathematics (STEM)
• Copyright Holders
• © 2012 The Authors
• Related URLs
• • http://uk.arxiv.org/abs/1210.1217(Other)
• Depositing User
• Carole Haswell