Independent discovery of the transiting exoplanet HAT-P-14b

E. K. Simpson; S. C. C. Barros; D. J. A. Brown; A. Collier Cameron; D. Pollacco; I. Skillen; H. C. Stempels; I. Boisse; F. Faedi; G. Hébrard; J. McCormac; P. Sorensen; R. A. Street; D. Anderson; J. Bento; F. Bouchy; O. W. Butters; B. Enoch; C. A. Haswell; L. Hebb; C. Hellier; S. Holmes; K. Horne; F. P. Keenan; T. A. Lister; P. F. L. Maxted; G. R. M. Miller; V. Moulds; C. Moutou; A. J. Norton; N. Parley; A. Santerne; B. Smalley; A. M. S. Smith; I. Todd; C. A. Watson; R. G. West; P. J. Wheatley

doi:10.1088/0004-6256/141/5/161

Independent discovery of the transiting exoplanet HAT-P-14b

E. K. Simpson, S. C. C. Barros, D. J. A. Brown, A. Collier Cameron, D. Pollacco, I. Skillen, H. C. Stempels, I. Boisse, F. Faedi, G. Hébrard, J. McCormac, P. Sorensen, R. A. Street, D. Anderson, J. Bento, F. Bouchy, O. W. Butters, B. Enoch, C. A. Haswell, L. HebbC. Hellier, S. Holmes, K. Horne, F. P. Keenan, T. A. Lister, P. F. L. Maxted, G. R. M. Miller, V. Moulds, C. Moutou, A. J. Norton, N. Parley, A. Santerne, B. Smalley, A. M. S. Smith, I. Todd, C. A. Watson, R. G. West, P. J. Wheatley

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9 Citations (Scopus)

Abstract

We present SuperWASP observations of HAT-P-14b, a hot Jupiter discovered by Torres et al. The planet was found independently by the SuperWASP team and named WASP-27b after follow-up observations had secured the discovery, but prior to the publication by Torres et al. Our analysis of HAT-P-14/WASP-27 is in good agreement with the values found by Torres et al. and we provide additional evidence against astronomical false positives. Due to the brightness of the host star, V_mag = 10, HAT-P-14b is an attractive candidate for further characterization observations. The planet has a high impact parameter and the primary transit is close to grazing. This could readily reveal small deviations in the orbital parameters indicating the presence of a third body in the system, which may be causing the small but significant orbital eccentricity. Our results suggest that the planet may undergo a grazing secondary eclipse. However, even a non-detection would tightly constrain the system parameters.

Original language	English
Article number	161
Pages (from-to)	1-7
Number of pages	7
Journal	Astronomical Journal
Volume	141
Issue number	5
DOIs	https://doi.org/10.1088/0004-6256/141/5/161
Publication status	Published - May 2011
Externally published	Yes

Keywords

planetary systems
stars: individual (HAT-P-14, WASP-27, GSC 3086-00152)
techniques: photometric
techniques: spectroscopic

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10.1088/0004-6256/141/5/161

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Simpson, E. K., Barros, S. C. C., Brown, D. J. A., Collier Cameron, A., Pollacco, D., Skillen, I., Stempels, H. C., Boisse, I., Faedi, F., Hébrard, G., McCormac, J., Sorensen, P., Street, R. A., Anderson, D., Bento, J., Bouchy, F., Butters, O. W., Enoch, B., Haswell, C. A., ... Wheatley, P. J. (2011). Independent discovery of the transiting exoplanet HAT-P-14b. Astronomical Journal, 141(5), 1-7. Article 161. https://doi.org/10.1088/0004-6256/141/5/161

@article{f6acbf4adf2c4cd9920bbf80c72a34e6,

title = "Independent discovery of the transiting exoplanet HAT-P-14b",

abstract = "We present SuperWASP observations of HAT-P-14b, a hot Jupiter discovered by Torres et al. The planet was found independently by the SuperWASP team and named WASP-27b after follow-up observations had secured the discovery, but prior to the publication by Torres et al. Our analysis of HAT-P-14/WASP-27 is in good agreement with the values found by Torres et al. and we provide additional evidence against astronomical false positives. Due to the brightness of the host star, Vmag = 10, HAT-P-14b is an attractive candidate for further characterization observations. The planet has a high impact parameter and the primary transit is close to grazing. This could readily reveal small deviations in the orbital parameters indicating the presence of a third body in the system, which may be causing the small but significant orbital eccentricity. Our results suggest that the planet may undergo a grazing secondary eclipse. However, even a non-detection would tightly constrain the system parameters.",

keywords = "planetary systems, stars: individual (HAT-P-14, WASP-27, GSC 3086-00152), techniques: photometric, techniques: spectroscopic",

author = "Simpson, \{E. K.\} and Barros, \{S. C. C.\} and Brown, \{D. J. A.\} and \{Collier Cameron\}, A. and D. Pollacco and I. Skillen and Stempels, \{H. C.\} and I. Boisse and F. Faedi and G. H{\'e}brard and J. McCormac and P. Sorensen and Street, \{R. A.\} and D. Anderson and J. Bento and F. Bouchy and Butters, \{O. W.\} and B. Enoch and Haswell, \{C. A.\} and L. Hebb and C. Hellier and S. Holmes and K. Horne and Keenan, \{F. P.\} and Lister, \{T. A.\} and Maxted, \{P. F. L.\} and Miller, \{G. R. M.\} and V. Moulds and C. Moutou and Norton, \{A. J.\} and N. Parley and A. Santerne and B. Smalley and Smith, \{A. M. S.\} and I. Todd and Watson, \{C. A.\} and West, \{R. G.\} and Wheatley, \{P. J.\}",

year = "2011",

month = may,

doi = "10.1088/0004-6256/141/5/161",

language = "English",

volume = "141",

pages = "1--7",

journal = "Astronomical Journal",

issn = "0004-6256",

publisher = "American Astronomical Society",

number = "5",

}

Simpson, EK, Barros, SCC, Brown, DJA, Collier Cameron, A, Pollacco, D, Skillen, I, Stempels, HC, Boisse, I, Faedi, F, Hébrard, G, McCormac, J, Sorensen, P, Street, RA, Anderson, D, Bento, J, Bouchy, F, Butters, OW, Enoch, B, Haswell, CA, Hebb, L, Hellier, C, Holmes, S, Horne, K, Keenan, FP, Lister, TA, Maxted, PFL, Miller, GRM, Moulds, V, Moutou, C, Norton, AJ, Parley, N, Santerne, A, Smalley, B, Smith, AMS, Todd, I, Watson, CA, West, RG & Wheatley, PJ 2011, 'Independent discovery of the transiting exoplanet HAT-P-14b', Astronomical Journal, vol. 141, no. 5, 161, pp. 1-7. https://doi.org/10.1088/0004-6256/141/5/161

TY - JOUR

T1 - Independent discovery of the transiting exoplanet HAT-P-14b

AU - Simpson, E. K.

AU - Barros, S. C. C.

AU - Brown, D. J. A.

AU - Collier Cameron, A.

AU - Pollacco, D.

AU - Skillen, I.

AU - Stempels, H. C.

AU - Boisse, I.

AU - Faedi, F.

AU - Hébrard, G.

AU - McCormac, J.

AU - Sorensen, P.

AU - Street, R. A.

AU - Anderson, D.

AU - Bento, J.

AU - Bouchy, F.

AU - Butters, O. W.

AU - Enoch, B.

AU - Haswell, C. A.

AU - Hebb, L.

AU - Hellier, C.

AU - Holmes, S.

AU - Horne, K.

AU - Keenan, F. P.

AU - Lister, T. A.

AU - Maxted, P. F. L.

AU - Miller, G. R. M.

AU - Moulds, V.

AU - Moutou, C.

AU - Norton, A. J.

AU - Parley, N.

AU - Santerne, A.

AU - Smalley, B.

AU - Smith, A. M. S.

AU - Todd, I.

AU - Watson, C. A.

AU - West, R. G.

AU - Wheatley, P. J.

PY - 2011/5

Y1 - 2011/5

N2 - We present SuperWASP observations of HAT-P-14b, a hot Jupiter discovered by Torres et al. The planet was found independently by the SuperWASP team and named WASP-27b after follow-up observations had secured the discovery, but prior to the publication by Torres et al. Our analysis of HAT-P-14/WASP-27 is in good agreement with the values found by Torres et al. and we provide additional evidence against astronomical false positives. Due to the brightness of the host star, Vmag = 10, HAT-P-14b is an attractive candidate for further characterization observations. The planet has a high impact parameter and the primary transit is close to grazing. This could readily reveal small deviations in the orbital parameters indicating the presence of a third body in the system, which may be causing the small but significant orbital eccentricity. Our results suggest that the planet may undergo a grazing secondary eclipse. However, even a non-detection would tightly constrain the system parameters.

AB - We present SuperWASP observations of HAT-P-14b, a hot Jupiter discovered by Torres et al. The planet was found independently by the SuperWASP team and named WASP-27b after follow-up observations had secured the discovery, but prior to the publication by Torres et al. Our analysis of HAT-P-14/WASP-27 is in good agreement with the values found by Torres et al. and we provide additional evidence against astronomical false positives. Due to the brightness of the host star, Vmag = 10, HAT-P-14b is an attractive candidate for further characterization observations. The planet has a high impact parameter and the primary transit is close to grazing. This could readily reveal small deviations in the orbital parameters indicating the presence of a third body in the system, which may be causing the small but significant orbital eccentricity. Our results suggest that the planet may undergo a grazing secondary eclipse. However, even a non-detection would tightly constrain the system parameters.

KW - planetary systems

KW - stars: individual (HAT-P-14, WASP-27, GSC 3086-00152)

KW - techniques: photometric

KW - techniques: spectroscopic

UR - https://www.scopus.com/pages/publications/79955651323

U2 - 10.1088/0004-6256/141/5/161

DO - 10.1088/0004-6256/141/5/161

M3 - Article

AN - SCOPUS:79955651323

SN - 0004-6256

VL - 141

SP - 1

EP - 7

JO - Astronomical Journal

JF - Astronomical Journal

IS - 5

M1 - 161

ER -

Independent discovery of the transiting exoplanet HAT-P-14b

Abstract

Keywords

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