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

M. Cappetta, R. P. Saglia, J. L. Birkby, J. Koppenhoefer, D. J. Pinfield, S. T. Hodgkin, P. Cruz, G. Kovács, B. Sipocz, D. Barrado, B. Nefs, Y. V. Pavlenko, L. Fossati, C. del Burgo, E. L. Martín, I. Snellen, J. Barnes, A. Bayo, D. A. Campbell, S. CatalanM. C. Gálvez-Ortiz, N. Goulding, C. Haswell, O. Ivanyuk, H. R. Jones, M. Kuznetsov, N. Lodieu, F. Marocco, Dimitrios Mislis, F. Murgas, R. Napiwotzki, E. Palle, D. Pollacco, L. Sarro Baro, E. Solano, P. Steele, H. Stoev, R. Tata, J. Zendejas

Research output: Contribution to journalArticle

17 Citations (Scopus)

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 1per cent to J ∼ 16 were constructed for ∼60000 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 3.35d, a planetary mass of 4.01 ± 0.35M J and a planetary radius of 1.49-0.18+0.16R J. WTS-1b has one of the largest radius anomalies among the known hot Jupiters in the mass range 3-5M J. The high irradiation from the host star ranks the planet in the pM class.

Original languageEnglish
Pages (from-to)1877-1890
Number of pages14
JournalMonthly Notices of the Royal Astronomical Society
Volume427
Issue number3
DOIs
Publication statusPublished - 11 Dec 2012
Externally publishedYes

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late stars
F stars
Jupiter (planet)
Jupiter
planets
planet
transit
orbits
stars
light curve
planetary mass
infrared telescopes
irradiation
United Kingdom
radii
extrasolar planets
anomaly
radial velocity
metallicity
time measurement

Keywords

  • Planetary systems
  • Planets and satellites: detection
  • Planets and satellites: individual: WTS1-b
  • Techniques: photometric
  • Techniques: radial velocities

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Cappetta, M., Saglia, R. P., Birkby, J. L., Koppenhoefer, J., Pinfield, D. J., Hodgkin, S. T., ... Zendejas, J. (2012). The first planet detected in the WTS: An inflated hot Jupiter in a 3.35d orbit around a late F star. Monthly Notices of the Royal Astronomical Society, 427(3), 1877-1890. https://doi.org/10.1111/j.1365-2966.2012.21937.x

The first planet detected in the WTS : An inflated hot Jupiter in a 3.35d 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.; Sipocz, B.; Barrado, D.; Nefs, B.; Pavlenko, Y. V.; Fossati, L.; del Burgo, C.; Martín, E. L.; Snellen, I.; Barnes, J.; Bayo, A.; Campbell, D. A.; Catalan, S.; Gálvez-Ortiz, M. C.; Goulding, N.; Haswell, C.; Ivanyuk, O.; Jones, H. R.; Kuznetsov, M.; Lodieu, N.; Marocco, F.; Mislis, Dimitrios; Murgas, F.; Napiwotzki, R.; Palle, E.; Pollacco, D.; Sarro Baro, L.; Solano, E.; Steele, P.; Stoev, H.; Tata, R.; Zendejas, J.

In: Monthly Notices of the Royal Astronomical Society, Vol. 427, No. 3, 11.12.2012, p. 1877-1890.

Research output: Contribution to journalArticle

Cappetta, M, Saglia, RP, Birkby, JL, Koppenhoefer, J, Pinfield, DJ, Hodgkin, ST, Cruz, P, Kovács, G, Sipocz, B, Barrado, D, Nefs, B, Pavlenko, YV, Fossati, L, del Burgo, C, Martín, EL, Snellen, I, Barnes, J, Bayo, A, Campbell, DA, Catalan, S, Gálvez-Ortiz, MC, Goulding, N, Haswell, C, Ivanyuk, O, Jones, HR, 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 & Zendejas, J 2012, 'The first planet detected in the WTS: An inflated hot Jupiter in a 3.35d orbit around a late F star', Monthly Notices of the Royal Astronomical Society, vol. 427, no. 3, pp. 1877-1890. https://doi.org/10.1111/j.1365-2966.2012.21937.x
Cappetta, M. ; Saglia, R. P. ; Birkby, J. L. ; Koppenhoefer, J. ; Pinfield, D. J. ; Hodgkin, S. T. ; Cruz, P. ; Kovács, G. ; Sipocz, B. ; Barrado, D. ; Nefs, B. ; Pavlenko, Y. V. ; Fossati, L. ; del Burgo, C. ; Martín, E. L. ; Snellen, I. ; Barnes, J. ; Bayo, A. ; Campbell, D. A. ; Catalan, S. ; Gálvez-Ortiz, M. C. ; Goulding, N. ; Haswell, C. ; Ivanyuk, O. ; Jones, H. R. ; Kuznetsov, M. ; Lodieu, N. ; Marocco, F. ; Mislis, Dimitrios ; Murgas, F. ; Napiwotzki, R. ; Palle, E. ; Pollacco, D. ; Sarro Baro, L. ; Solano, E. ; Steele, P. ; Stoev, H. ; Tata, R. ; Zendejas, J. / The first planet detected in the WTS : An inflated hot Jupiter in a 3.35d orbit around a late F star. In: Monthly Notices of the Royal Astronomical Society. 2012 ; Vol. 427, No. 3. pp. 1877-1890.
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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 1per cent to J ∼ 16 were constructed for ∼60000 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 3.35d, a planetary mass of 4.01 ± 0.35M J and a planetary radius of 1.49-0.18+0.16R J. WTS-1b has one of the largest radius anomalies among the known hot Jupiters in the mass range 3-5M J. The high irradiation from the host star ranks the planet in the pM class.",
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T1 - The first planet detected in the WTS

T2 - An inflated hot Jupiter in a 3.35d orbit around a late F star

AU - Cappetta, M.

AU - Saglia, R. P.

AU - Birkby, J. L.

AU - Koppenhoefer, J.

AU - Pinfield, D. J.

AU - Hodgkin, S. T.

AU - Cruz, P.

AU - Kovács, G.

AU - Sipocz, B.

AU - Barrado, D.

AU - Nefs, B.

AU - Pavlenko, Y. V.

AU - Fossati, L.

AU - del Burgo, C.

AU - Martín, E. L.

AU - Snellen, I.

AU - Barnes, J.

AU - Bayo, A.

AU - Campbell, D. A.

AU - Catalan, S.

AU - Gálvez-Ortiz, M. C.

AU - Goulding, N.

AU - Haswell, C.

AU - Ivanyuk, O.

AU - Jones, H. R.

AU - Kuznetsov, M.

AU - Lodieu, N.

AU - Marocco, F.

AU - Mislis, Dimitrios

AU - Murgas, F.

AU - Napiwotzki, R.

AU - Palle, E.

AU - Pollacco, D.

AU - Sarro Baro, L.

AU - Solano, E.

AU - Steele, P.

AU - Stoev, H.

AU - Tata, R.

AU - Zendejas, J.

PY - 2012/12/11

Y1 - 2012/12/11

N2 - 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 1per cent to J ∼ 16 were constructed for ∼60000 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 3.35d, a planetary mass of 4.01 ± 0.35M J and a planetary radius of 1.49-0.18+0.16R J. WTS-1b has one of the largest radius anomalies among the known hot Jupiters in the mass range 3-5M J. The high irradiation from the host star ranks the planet in the pM class.

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KW - Planetary systems

KW - Planets and satellites: detection

KW - Planets and satellites: individual: WTS1-b

KW - Techniques: photometric

KW - Techniques: radial velocities

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