New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South

Coel Hellier; D. R.  Andrerson; F. Bouchy; A. Burdanov; A. Collier Cameron; L. Delrez; M. Gillon; E. Jehin; M. Lendl; L. D. Nielsen; P. F. L. Maxted; F. Pepe; D. Pollacco; D. Queloz; D. Ségransan; B. Smalley; A. H. M. J. Triaud; S. Udry; R. G. West

doi:10.1093/mnras/sty2741

New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South

Coel Hellier, D. R. Andrerson, F. Bouchy, A. Burdanov, A. Collier Cameron, L. Delrez, M. Gillon, E. Jehin, M. Lendl, L. D. Nielsen, P. F. L. Maxted, F. Pepe, D. Pollacco, D. Queloz, D. Ségransan, B. Smalley, A. H. M. J. Triaud, S. Udry, R. G. West

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

Abstract

We report the discovery of eight hot-Jupiter exoplanets from the WASP-South transit survey. WASP-144b has a mass of 0.44 M_Jup, a radius of 0.85 R_Jup, and is in a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational modulation. WASP-145Ab is a 0.89 M_Jup planet in a 1.77-d orbit with a grazing transit. The host is a V = 11.5, K2 star with a companion 5 arcsec away and 1.4 mag fainter. WASP-158b is a relatively massive planet at 2.8 M_Jup with a radius of 1.1 R_Jup and a 3.66-d orbit. It transits a V = 12.1, F6 star. WASP-159b is a bloated hot Jupiter (1.4 R_Jup and 0.55 M_Jup) in a 3.8-d orbit around a V = 12.9, F9 star. WASP-162b is a massive planet in a relatively long and highly eccentric orbit (5.2 M_Jup, P = 9.6 d, e = 0.43). It transits a V = 12.2, K0 star. WASP-168b is a bloated hot Jupiter (0.42 M_Jup; 1.5 R_Jup) in a 4.15-d orbit with a grazing transit. The host is a V = 12.1, F9 star. WASP-172b is a bloated hot Jupiter (0.5 M_Jup; 1.6 R_Jup) in a 5.48-d orbit around a V = 11.0, F1 star. WASP-173Ab is a massive planet (3.7 M_Jup) with a 1.2 R_Jup radius in a circular orbit with a period of 1.39 d. The host is a V = 11.3, G3 star, being the brighter component of the double-star system WDS23366 − 3437, with a companion 6 arcsec away and 0.8 mag fainter. One of the two stars shows a rotational modulation of 7.9 d.

Original language	English
Pages (from-to)	1379-1391
Number of pages	13
Journal	Monthly Notices of the Royal Astronomical Society
Volume	482
Issue number	1
Early online date	9 Oct 2018
DOIs	https://doi.org/10.1093/mnras/sty2741
Publication status	Published - 1 Jan 2019

Keywords

Stars: individual (WASP-144, WASP-145A, WASP-158, WASP-159, WASP-162, WASP-168, WASP-172, WASP-173A)
Planetary systems

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10.1093/mnras/sty2741

Hellier_2018_MNRAS_Newtransiting_FinalPubVersion
Copyright © 2018 The Author(s) Published by Oxford University Press on behalf of the Royal Astronomical Society. This work is made available online in accordance with the publisher’s policies. This is the final published version of the work, which was originally published at: https://doi.org/10.1093/mnras/sty2741
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http://adsabs.harvard.edu/abs/2019MNRAS.482.1379H

Astronomy at St Andrews 2018-2021: Astronomy at St Andrews 2018-2021
Jardine, M. M. (PI), Bonnell, I. A. (CoI), Cameron, A. C. (CoI), Cyganowski, C. J. (CoI), Dominik, M. (CoI), Helling, C. (CoI), Horne, K. D. (CoI), Scholz, A. (CoI), Tojeiro, R. (CoI), Weijmans, A.-M. (CoI), Wild, V. (CoI), Woitke, P. (CoI), Wood, K. (CoI) & Zhao, H. (CoI)
1/04/18 → 31/03/22
Project: Standard
Support for the PLATO Development: Support for the PLATO Development Phase 2017-2022: Planet candidate ranking and validation
Cameron, A. C. (PI)
Science & Technology Facilities Council
1/08/17 → 31/12/22
Project: Standard
Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018
Jardine, M. M. (PI), Cameron, A. C. (CoI), Cyganowski, C. J. (CoI), Horne, K. D. (CoI) & Wood, K. (CoI)
Science & Technology Facilities Council
1/04/15 → 31/03/18
Project: Standard

Cite this

Hellier, C., Andrerson, D. R., Bouchy, F., Burdanov, A., Cameron, A. C., Delrez, L., Gillon, M., Jehin, E., Lendl, M., Nielsen, L. D., Maxted, P. F. L., Pepe, F., Pollacco, D., Queloz, D., Ségransan, D., Smalley, B., Triaud, A. H. M. J., Udry, S., & West, R. G. (2019). New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South. Monthly Notices of the Royal Astronomical Society, 482(1), 1379-1391. https://doi.org/10.1093/mnras/sty2741

@article{bbe5f6cd555749ceb2e57a6c7348a785,

title = "New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South",

abstract = "We report the discovery of eight hot-Jupiter exoplanets from the WASP-South transit survey. WASP-144b has a mass of 0.44 MJup, a radius of 0.85 RJup, and is in a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational modulation. WASP-145Ab is a 0.89 MJup planet in a 1.77-d orbit with a grazing transit. The host is a V = 11.5, K2 star with a companion 5 arcsec away and 1.4 mag fainter. WASP-158b is a relatively massive planet at 2.8 MJup with a radius of 1.1 RJup and a 3.66-d orbit. It transits a V = 12.1, F6 star. WASP-159b is a bloated hot Jupiter (1.4 RJup and 0.55 MJup) in a 3.8-d orbit around a V = 12.9, F9 star. WASP-162b is a massive planet in a relatively long and highly eccentric orbit (5.2 MJup, P = 9.6 d, e = 0.43). It transits a V = 12.2, K0 star. WASP-168b is a bloated hot Jupiter (0.42 MJup; 1.5 RJup) in a 4.15-d orbit with a grazing transit. The host is a V = 12.1, F9 star. WASP-172b is a bloated hot Jupiter (0.5 MJup; 1.6 RJup) in a 5.48-d orbit around a V = 11.0, F1 star. WASP-173Ab is a massive planet (3.7 MJup) with a 1.2 RJup radius in a circular orbit with a period of 1.39 d. The host is a V = 11.3, G3 star, being the brighter component of the double-star system WDS23366 − 3437, with a companion 6 arcsec away and 0.8 mag fainter. One of the two stars shows a rotational modulation of 7.9 d.",

keywords = "Stars: individual (WASP-144, WASP-145A, WASP-158, WASP-159, WASP-162, WASP-168, WASP-172, WASP-173A), Planetary systems",

author = "Coel Hellier and Andrerson, {D. R.} and F. Bouchy and A. Burdanov and Cameron, {A. Collier} and L. Delrez and M. Gillon and E. Jehin and M. Lendl and Nielsen, {L. D.} and Maxted, {P. F. L.} and F. Pepe and D. Pollacco and D. Queloz and D. S{\'e}gransan and B. Smalley and Triaud, {A. H. M. J.} and S. Udry and West, {R. G.}",

note = "Funding for WASP comes from consortium universities and from the UK{\textquoteright}s Science and Technology Facilities Council. The Euler Swiss telescope is supported by the Swiss National Science Foundation. TRAPPIST-South is funded by the Belgian Fund for Scientific Research (Fond National de la Recherche Scientifique, FNRS) under the grant FRFC 2.5.594.09.F, with the participation of the Swiss National Science Fundation (SNF).The research leading to these results has received funding from the ARC grant for Concerted Research Actions, financed by the Wallonia-Brussels Federation. MG and EJ are, respectively, Research Associate and Senior Research Associate at the FNRS-F.R.S. LD acknowledges support from a Gruber Foundation Fellowship.",

year = "2019",

month = jan,

day = "1",

doi = "10.1093/mnras/sty2741",

language = "English",

volume = "482",

pages = "1379--1391",

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

issn = "0035-8711",

publisher = "Oxford University Press",

number = "1",

}

Hellier, C, Andrerson, DR, Bouchy, F, Burdanov, A, Cameron, AC, Delrez, L, Gillon, M, Jehin, E, Lendl, M, Nielsen, LD, Maxted, PFL, Pepe, F, Pollacco, D, Queloz, D, Ségransan, D, Smalley, B, Triaud, AHMJ, Udry, S & West, RG 2019, 'New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South', Monthly Notices of the Royal Astronomical Society, vol. 482, no. 1, pp. 1379-1391. https://doi.org/10.1093/mnras/sty2741

TY - JOUR

T1 - New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South

AU - Hellier, Coel

AU - Andrerson, D. R.

AU - Bouchy, F.

AU - Burdanov, A.

AU - Cameron, A. Collier

AU - Delrez, L.

AU - Gillon, M.

AU - Jehin, E.

AU - Lendl, M.

AU - Nielsen, L. D.

AU - Maxted, P. F. L.

AU - Pepe, F.

AU - Pollacco, D.

AU - Queloz, D.

AU - Ségransan, D.

AU - Smalley, B.

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

AU - Udry, S.

AU - West, R. G.

N1 - Funding for WASP comes from consortium universities and from the UK’s Science and Technology Facilities Council. The Euler Swiss telescope is supported by the Swiss National Science Foundation. TRAPPIST-South is funded by the Belgian Fund for Scientific Research (Fond National de la Recherche Scientifique, FNRS) under the grant FRFC 2.5.594.09.F, with the participation of the Swiss National Science Fundation (SNF).The research leading to these results has received funding from the ARC grant for Concerted Research Actions, financed by the Wallonia-Brussels Federation. MG and EJ are, respectively, Research Associate and Senior Research Associate at the FNRS-F.R.S. LD acknowledges support from a Gruber Foundation Fellowship.

PY - 2019/1/1

Y1 - 2019/1/1

N2 - We report the discovery of eight hot-Jupiter exoplanets from the WASP-South transit survey. WASP-144b has a mass of 0.44 MJup, a radius of 0.85 RJup, and is in a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational modulation. WASP-145Ab is a 0.89 MJup planet in a 1.77-d orbit with a grazing transit. The host is a V = 11.5, K2 star with a companion 5 arcsec away and 1.4 mag fainter. WASP-158b is a relatively massive planet at 2.8 MJup with a radius of 1.1 RJup and a 3.66-d orbit. It transits a V = 12.1, F6 star. WASP-159b is a bloated hot Jupiter (1.4 RJup and 0.55 MJup) in a 3.8-d orbit around a V = 12.9, F9 star. WASP-162b is a massive planet in a relatively long and highly eccentric orbit (5.2 MJup, P = 9.6 d, e = 0.43). It transits a V = 12.2, K0 star. WASP-168b is a bloated hot Jupiter (0.42 MJup; 1.5 RJup) in a 4.15-d orbit with a grazing transit. The host is a V = 12.1, F9 star. WASP-172b is a bloated hot Jupiter (0.5 MJup; 1.6 RJup) in a 5.48-d orbit around a V = 11.0, F1 star. WASP-173Ab is a massive planet (3.7 MJup) with a 1.2 RJup radius in a circular orbit with a period of 1.39 d. The host is a V = 11.3, G3 star, being the brighter component of the double-star system WDS23366 − 3437, with a companion 6 arcsec away and 0.8 mag fainter. One of the two stars shows a rotational modulation of 7.9 d.

AB - We report the discovery of eight hot-Jupiter exoplanets from the WASP-South transit survey. WASP-144b has a mass of 0.44 MJup, a radius of 0.85 RJup, and is in a 2.27-d orbit around a V = 12.9, K2 star which shows a 21-d rotational modulation. WASP-145Ab is a 0.89 MJup planet in a 1.77-d orbit with a grazing transit. The host is a V = 11.5, K2 star with a companion 5 arcsec away and 1.4 mag fainter. WASP-158b is a relatively massive planet at 2.8 MJup with a radius of 1.1 RJup and a 3.66-d orbit. It transits a V = 12.1, F6 star. WASP-159b is a bloated hot Jupiter (1.4 RJup and 0.55 MJup) in a 3.8-d orbit around a V = 12.9, F9 star. WASP-162b is a massive planet in a relatively long and highly eccentric orbit (5.2 MJup, P = 9.6 d, e = 0.43). It transits a V = 12.2, K0 star. WASP-168b is a bloated hot Jupiter (0.42 MJup; 1.5 RJup) in a 4.15-d orbit with a grazing transit. The host is a V = 12.1, F9 star. WASP-172b is a bloated hot Jupiter (0.5 MJup; 1.6 RJup) in a 5.48-d orbit around a V = 11.0, F1 star. WASP-173Ab is a massive planet (3.7 MJup) with a 1.2 RJup radius in a circular orbit with a period of 1.39 d. The host is a V = 11.3, G3 star, being the brighter component of the double-star system WDS23366 − 3437, with a companion 6 arcsec away and 0.8 mag fainter. One of the two stars shows a rotational modulation of 7.9 d.

KW - Stars: individual (WASP-144, WASP-145A, WASP-158, WASP-159, WASP-162, WASP-168, WASP-172, WASP-173A)

KW - Planetary systems

U2 - 10.1093/mnras/sty2741

DO - 10.1093/mnras/sty2741

M3 - Article

SN - 0035-8711

VL - 482

SP - 1379

EP - 1391

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

New transiting hot Jupiters discovered by WASP-South, Euler/CORALIE, and TRAPPIST-South

Abstract

Keywords

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Astronomy at St Andrews 2018-2021: Astronomy at St Andrews 2018-2021

Support for the PLATO Development: Support for the PLATO Development Phase 2017-2022: Planet candidate ranking and validation

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

Cite this