WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets

K. L. Hay; Andrew Collier Cameron; A. P. Doyle; G. Hébrard; I. Skillen; D. R. Anderson; S. C. C. Barros; D. J. A. Brown; F. Bouchy; R. Busuttil; P. Delorme; L. Delrez; O. Demangeon; R. F. Díaz; M. Gillon; E. Gonzàlez; C. Hellier; S. Holmes; J. F. Jarvis; E. Jehin; Y. C. Joshi; U. Kolb; M. Lendl; P. F. L. Maxted; J. McCormac; G. R. M. Miller; A. Mortier; D. Pollacco; D. Queloz; D. Ségransan; E. K. Simpson; B. Smalley; J. Southworth; A. H. M. J. Triaud; O. D. Turner; S. Udry; M. Vanhuysse; R. G. West; P. A. Wilson

doi:10.1093/mnras/stw2090

WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets

K. L. Hay
, Andrew Collier Cameron
, A. P. Doyle
, G. Hébrard
, I. Skillen
, D. R. Anderson
, S. C. C. Barros
, D. J. A. Brown
, F. Bouchy
, R. Busuttil
, P. Delorme
, L. Delrez
, O. Demangeon
, R. F. Díaz
, M. Gillon
, E. Gonzàlez
, C. Hellier
, S. Holmes
, J. F. Jarvis
, E. Jehin

Y. C. Joshi, U. Kolb, M. Lendl, P. F. L. Maxted, J. McCormac, G. R. M. Miller, A. Mortier, D. Pollacco, D. Queloz, D. Ségransan, E. K. Simpson, B. Smalley, J. Southworth, A. H. M. J. Triaud, O. D. Turner, S. Udry, M. Vanhuysse, R. G. West, P. A. Wilson

School of Physics and Astronomy

Research output: Contribution to journal › Article › peer-review

Abstract

We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground-based photometric lightcurves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 days, which has R_p = 1.461 ± 0.077R_J and M_p = 0.805 ± 0.068M_J. WASP-93b orbits its F4 host star every 2.73 days and has R_p = 1.597 ± 0.077R_J and M_p = 1.47 ± 0.029M_J. WASP-118b also has a hot host star (F6) and is moderately inflated, where R_p = 1.440 ± 0.036R_J and Mp = 0.513 ± 0.041M_J and the planet has an orbital period of 4.05 days. They are bright targets (V = 13.18, 10.97 and 11.07 respectively) ideal for further characterisation work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. WASP-93b is expected to be tidally migrating outwards, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.

Original language	English
Pages (from-to)	3276-3289
Number of pages	14
Journal	Monthly Notices of the Royal Astronomical Society
Volume	463
Issue number	3
Early online date	24 Aug 2016
DOIs	https://doi.org/10.1093/mnras/stw2090
Publication status	Published - 11 Dec 2016

Keywords

Techniques: photometric
Techniques: radial velocities
Planets and satellites: detection
Planet-star interactions
Planetary systems

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10.1093/mnras/stw2090

Hay_2016_WASP-92b_MNRAS_AAM
© 2016, the Author(s). This work is made available online in accordance with the publisher’s policies. This is the author created, accepted version manuscript following peer review and may differ slightly from the final published version. The final published version of this work is available at https://dx.doi.org/10.1093/mnras/stw2090
Accepted author manuscript, 3.51 MB

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Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018
Jardine, M. (PI), Cameron, A. (CoI), Cyganowski, C. (CoI), Horne, K. (CoI) & Wood, K. (CoI)
Science & Technology Facilities Council
1/04/15 → 31/03/18
Project: Standard
PATT linked Travel and Subsistence: St Andrrews Astronomy PATT linked Travel and subsistence
Cameron, A. (PI), Driver, S. (CoI), Greaves, J. (CoI) & Horne, K. (CoI)
Science & Technology Facilities Council
1/10/10 → 30/09/13
Project: Standard
PATT Linked Travel ST/G001006/1: Patt Linked Travel & Subsistence
Cameron, A. (PI), Driver, S. (CoI), Greaves, J. (CoI) & Horne, K. (CoI)
Science & Technology Facilities Council
1/10/08 → 30/09/10
Project: Standard

Cite this

Hay, K. L., Cameron, A. C., Doyle, A. P., Hébrard, G., Skillen, I., Anderson, D. R., Barros, S. C. C., Brown, D. J. A., Bouchy, F., Busuttil, R., Delorme, P., Delrez, L., Demangeon, O., Díaz, R. F., Gillon, M., Gonzàlez, E., Hellier, C., Holmes, S., Jarvis, J. F., ... Wilson, P. A. (2016). WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets. Monthly Notices of the Royal Astronomical Society, 463(3), 3276-3289. https://doi.org/10.1093/mnras/stw2090

@article{2ea23bd46ced42b4aeb5bdf9a45994a1,

title = "WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets",

abstract = "We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground-based photometric lightcurves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 days, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 days and has Rp = 1.597 ± 0.077RJ and Mp = 1.47 ± 0.029MJ. WASP-118b also has a hot host star (F6) and is moderately inflated, where Rp = 1.440 ± 0.036RJ and Mp = 0.513 ± 0.041MJ and the planet has an orbital period of 4.05 days. They are bright targets (V = 13.18, 10.97 and 11.07 respectively) ideal for further characterisation work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. WASP-93b is expected to be tidally migrating outwards, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.",

keywords = "Techniques: photometric, Techniques: radial velocities, Planets and satellites: detection, Planet-star interactions, Planetary systems",

author = "Hay, \{K. L.\} and Cameron, \{Andrew Collier\} and Doyle, \{A. P.\} and G. H{\'e}brard and I. Skillen and Anderson, \{D. R.\} and Barros, \{S. C. C.\} and Brown, \{D. J. A.\} and F. Bouchy and R. Busuttil and P. Delorme and L. Delrez and O. Demangeon and D{\'i}az, \{R. F.\} and M. Gillon and E. Gonz{\`a}lez and C. Hellier and S. Holmes and Jarvis, \{J. F.\} and E. Jehin and Joshi, \{Y. C.\} and U. Kolb and M. Lendl and Maxted, \{P. F. L.\} and J. McCormac and Miller, \{G. R. M.\} and A. Mortier and D. Pollacco and D. Queloz and D. S{\'e}gransan and Simpson, \{E. K.\} and B. Smalley and J. Southworth and Triaud, \{A. H. M. J.\} and Turner, \{O. D.\} and S. Udry and M. Vanhuysse and West, \{R. G.\} and Wilson, \{P. A.\}",

note = "KH and ACC acknowledge support from STFC doctoral training grant ST/M503812/1 and grant ST/M001296/1 respectively. The research leading to these results has received funding from the European Community{\textquoteright}s Seventh Framework Programme (FP7/2013-2016) under grant agreement number 312430 (OPTICON).",

year = "2016",

month = dec,

day = "11",

doi = "10.1093/mnras/stw2090",

language = "English",

volume = "463",

pages = "3276--3289",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "3",

}

Hay, KL, Cameron, AC, Doyle, AP, Hébrard, G, Skillen, I, Anderson, DR, Barros, SCC, Brown, DJA, Bouchy, F, Busuttil, R, Delorme, P, Delrez, L, Demangeon, O, Díaz, RF, Gillon, M, Gonzàlez, E, Hellier, C, Holmes, S, Jarvis, JF, Jehin, E, Joshi, YC, Kolb, U, Lendl, M, Maxted, PFL, McCormac, J, Miller, GRM, Mortier, A, Pollacco, D, Queloz, D, Ségransan, D, Simpson, EK, Smalley, B, Southworth, J, Triaud, AHMJ, Turner, OD, Udry, S, Vanhuysse, M, West, RG & Wilson, PA 2016, 'WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets', Monthly Notices of the Royal Astronomical Society, vol. 463, no. 3, pp. 3276-3289. https://doi.org/10.1093/mnras/stw2090

TY - JOUR

T1 - WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets

AU - Hay, K. L.

AU - Cameron, Andrew Collier

AU - Doyle, A. P.

AU - Hébrard, G.

AU - Skillen, I.

AU - Anderson, D. R.

AU - Barros, S. C. C.

AU - Brown, D. J. A.

AU - Bouchy, F.

AU - Busuttil, R.

AU - Delorme, P.

AU - Delrez, L.

AU - Demangeon, O.

AU - Díaz, R. F.

AU - Gillon, M.

AU - Gonzàlez, E.

AU - Hellier, C.

AU - Holmes, S.

AU - Jarvis, J. F.

AU - Jehin, E.

AU - Joshi, Y. C.

AU - Kolb, U.

AU - Lendl, M.

AU - Maxted, P. F. L.

AU - McCormac, J.

AU - Miller, G. R. M.

AU - Mortier, A.

AU - Pollacco, D.

AU - Queloz, D.

AU - Ségransan, D.

AU - Simpson, E. K.

AU - Smalley, B.

AU - Southworth, J.

AU - Triaud, A. H. M. J.

AU - Turner, O. D.

AU - Udry, S.

AU - Vanhuysse, M.

AU - West, R. G.

AU - Wilson, P. A.

N1 - KH and ACC acknowledge support from STFC doctoral training grant ST/M503812/1 and grant ST/M001296/1 respectively. The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2013-2016) under grant agreement number 312430 (OPTICON).

PY - 2016/12/11

Y1 - 2016/12/11

N2 - We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground-based photometric lightcurves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 days, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 days and has Rp = 1.597 ± 0.077RJ and Mp = 1.47 ± 0.029MJ. WASP-118b also has a hot host star (F6) and is moderately inflated, where Rp = 1.440 ± 0.036RJ and Mp = 0.513 ± 0.041MJ and the planet has an orbital period of 4.05 days. They are bright targets (V = 13.18, 10.97 and 11.07 respectively) ideal for further characterisation work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. WASP-93b is expected to be tidally migrating outwards, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.

AB - We present the discovery of three new transiting giant planets, first detected with the WASP telescopes, and establish their planetary nature with follow up spectroscopy and ground-based photometric lightcurves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 days, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 days and has Rp = 1.597 ± 0.077RJ and Mp = 1.47 ± 0.029MJ. WASP-118b also has a hot host star (F6) and is moderately inflated, where Rp = 1.440 ± 0.036RJ and Mp = 0.513 ± 0.041MJ and the planet has an orbital period of 4.05 days. They are bright targets (V = 13.18, 10.97 and 11.07 respectively) ideal for further characterisation work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. WASP-93b is expected to be tidally migrating outwards, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.

KW - Techniques: photometric

KW - Techniques: radial velocities

KW - Planets and satellites: detection

KW - Planet-star interactions

KW - Planetary systems

U2 - 10.1093/mnras/stw2090

DO - 10.1093/mnras/stw2090

M3 - Article

SN - 0035-8711

VL - 463

SP - 3276

EP - 3289

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -

WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets

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Keywords

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Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018

PATT linked Travel and Subsistence: St Andrrews Astronomy PATT linked Travel and subsistence

PATT Linked Travel ST/G001006/1: Patt Linked Travel & Subsistence

Cite this