WASP-147b, 160Bb, 164b and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts

M. Lendl; D. R. Anderson; A. Bonfanti; F. Bouchy; A. Burdanov; A. Collier Cameron; L. Delrez; M. Gillon; C. Hellier; E. Jehin; P. F. L. Maxted; L. Dyregaard Nielsen; F. Pepe; D. Pollacco; D. Queloz; D. Segransan; J. Southworth; B. Smalley; S. Thompson; O. Turner; A. H. M. J. Triaud; S. Udry; R. G. West

doi:10.1093/mnras/sty2667

WASP-147b, 160Bb, 164b and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts

M. Lendl
, D. R. Anderson
, A. Bonfanti
, F. Bouchy
, A. Burdanov
, A. Collier Cameron
, L. Delrez
, M. Gillon
, C. Hellier
, E. Jehin
, P. F. L. Maxted
, L. Dyregaard Nielsen
, F. Pepe
, D. Pollacco
, D. Queloz
, D. Segransan
, J. Southworth
, B. Smalley
, S. Thompson
, O. Turner

A. H. M. J. Triaud, S. Udry, R. G. West

Physics and Astronomy

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

5 Citations (Scopus)

142 Downloads (Pure)

Abstract

We report the discovery of four transiting hot Jupiters, WASP-147, WASP-160B, WASP-164, and WASP-165 from the WASP survey. WASP-147b is a near Saturn-mass (MP = 0.28MJ) object with a radius of 1.11R_J orbiting a G4 star with a period of 4.6 d. WASP-160Bb has a mass and radius (⁠M_p=0.28M_J⁠, R_p=1.09R_J⁠) near-identical to WASP-147b, but is less irradiated, orbiting a metal-rich ([Fe/H]* = 0.27) K0 star with a period of 3.8 d. WASP-160B is part of a near equal-mass visual binary with an on-sky separation of 28.5 arcsec. WASP-164b is a more massive (⁠M_P=2.13M_J⁠, R_p=1.13R_J⁠) hot Jupiter, orbiting a G2 star on a close-in (P = 1.8 d), but tidally stable orbit. WASP-165b is a classical (⁠M_p=0.66M_J⁠, R_P=1.26R_J⁠) hot Jupiter in a 3.5 d period orbit around a metal-rich ([Fe/H]* = 0.33) star. WASP-147b and WASP-160Bb are promising targets for atmospheric characterization through transmission spectroscopy, while WASP-164b presents a good target for emission spectroscopy.

Original language	English
Pages (from-to)	301–312
Number of pages	12
Journal	Monthly Notices of the Royal Astronomical Society
Volume	482
Issue number	1
Early online date	3 Oct 2018
DOIs	https://doi.org/10.1093/mnras/sty2667
Publication status	Published - 1 Jan 2019

Bibliographical note

published in MNRAS

Keywords

astro-ph.EP
planets and satellites: detection
planetary systems

Access to Document

10.1093/mnras/sty2667Licence: None: All rights reserved

M._Lendl_et_al_WASP_147b,_160Bb,_164b_and_165b_Monthly_Notices_of_the_Royal_Astronomical_Society_2018
Checked for eligibility: 12/07/2019 This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2018 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. https://doi.org/10.1093/mnras/sty2667
Final published version, 1.41 MBLicence: None: All rights reserved

http://arxiv.org/abs/1807.06973v2Licence: None: All rights reserved

Cite this

Lendl, M., Anderson, D. R., Bonfanti, A., Bouchy, F., Burdanov, A., Cameron, A. C., Delrez, L., Gillon, M., Hellier, C., Jehin, E., Maxted, P. F. L., Nielsen, L. D., Pepe, F., Pollacco, D., Queloz, D., Segransan, D., Southworth, J., Smalley, B., Thompson, S., ... West, R. G. (2019). WASP-147b, 160Bb, 164b and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts. Monthly Notices of the Royal Astronomical Society, 482(1), 301–312. https://doi.org/10.1093/mnras/sty2667

@article{d7d0929b2f284e70899a6c92f11e8cdb,

title = "WASP-147b, 160Bb, 164b and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts",

abstract = "We report the discovery of four transiting hot Jupiters, WASP-147, WASP-160B, WASP-164, and WASP-165 from the WASP survey. WASP-147b is a near Saturn-mass (MP = 0.28MJ) object with a radius of 1.11RJ orbiting a G4 star with a period of 4.6 d. WASP-160Bb has a mass and radius (⁠Mp=0.28MJ⁠, Rp=1.09RJ⁠) near-identical to WASP-147b, but is less irradiated, orbiting a metal-rich ([Fe/H]* = 0.27) K0 star with a period of 3.8 d. WASP-160B is part of a near equal-mass visual binary with an on-sky separation of 28.5 arcsec. WASP-164b is a more massive (⁠MP=2.13MJ⁠, Rp=1.13RJ⁠) hot Jupiter, orbiting a G2 star on a close-in (P = 1.8 d), but tidally stable orbit. WASP-165b is a classical (⁠Mp=0.66MJ⁠, RP=1.26RJ⁠) hot Jupiter in a 3.5 d period orbit around a metal-rich ([Fe/H]* = 0.33) star. WASP-147b and WASP-160Bb are promising targets for atmospheric characterization through transmission spectroscopy, while WASP-164b presents a good target for emission spectroscopy.",

keywords = "astro-ph.EP, planets and satellites: detection, planetary systems",

author = "M. Lendl and Anderson, \{D. R.\} and A. Bonfanti and F. Bouchy and A. Burdanov and Cameron, \{A. Collier\} and L. Delrez and M. Gillon and C. Hellier and E. Jehin and Maxted, \{P. F. L.\} and Nielsen, \{L. Dyregaard\} and F. Pepe and D. Pollacco and D. Queloz and D. Segransan and J. Southworth and B. Smalley and S. Thompson and O. Turner and Triaud, \{A. H. M. J.\} and S. Udry and West, \{R. G.\}",

note = "published in MNRAS",

year = "2019",

month = jan,

day = "1",

doi = "10.1093/mnras/sty2667",

language = "English",

volume = "482",

pages = "301–312",

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

issn = "0035-8711",

publisher = "SIPRI/Oxford University Press",

number = "1",

}

Lendl, M, Anderson, DR, Bonfanti, A, Bouchy, F, Burdanov, A, Cameron, AC, Delrez, L, Gillon, M, Hellier, C, Jehin, E, Maxted, PFL, Nielsen, LD, Pepe, F, Pollacco, D, Queloz, D, Segransan, D, Southworth, J, Smalley, B, Thompson, S, Turner, O, Triaud, AHMJ, Udry, S & West, RG 2019, 'WASP-147b, 160Bb, 164b and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts', Monthly Notices of the Royal Astronomical Society, vol. 482, no. 1, pp. 301–312. https://doi.org/10.1093/mnras/sty2667

TY - JOUR

T1 - WASP-147b, 160Bb, 164b and 165b

T2 - two hot Saturns and two Jupiters, including two planets with metal-rich hosts

AU - Lendl, M.

AU - Anderson, D. R.

AU - Bonfanti, A.

AU - Bouchy, F.

AU - Burdanov, A.

AU - Cameron, A. Collier

AU - Delrez, L.

AU - Gillon, M.

AU - Hellier, C.

AU - Jehin, E.

AU - Maxted, P. F. L.

AU - Nielsen, L. Dyregaard

AU - Pepe, F.

AU - Pollacco, D.

AU - Queloz, D.

AU - Segransan, D.

AU - Southworth, J.

AU - Smalley, B.

AU - Thompson, S.

AU - Turner, O.

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

AU - Udry, S.

AU - West, R. G.

N1 - published in MNRAS

PY - 2019/1/1

Y1 - 2019/1/1

N2 - We report the discovery of four transiting hot Jupiters, WASP-147, WASP-160B, WASP-164, and WASP-165 from the WASP survey. WASP-147b is a near Saturn-mass (MP = 0.28MJ) object with a radius of 1.11RJ orbiting a G4 star with a period of 4.6 d. WASP-160Bb has a mass and radius (⁠Mp=0.28MJ⁠, Rp=1.09RJ⁠) near-identical to WASP-147b, but is less irradiated, orbiting a metal-rich ([Fe/H]* = 0.27) K0 star with a period of 3.8 d. WASP-160B is part of a near equal-mass visual binary with an on-sky separation of 28.5 arcsec. WASP-164b is a more massive (⁠MP=2.13MJ⁠, Rp=1.13RJ⁠) hot Jupiter, orbiting a G2 star on a close-in (P = 1.8 d), but tidally stable orbit. WASP-165b is a classical (⁠Mp=0.66MJ⁠, RP=1.26RJ⁠) hot Jupiter in a 3.5 d period orbit around a metal-rich ([Fe/H]* = 0.33) star. WASP-147b and WASP-160Bb are promising targets for atmospheric characterization through transmission spectroscopy, while WASP-164b presents a good target for emission spectroscopy.

AB - We report the discovery of four transiting hot Jupiters, WASP-147, WASP-160B, WASP-164, and WASP-165 from the WASP survey. WASP-147b is a near Saturn-mass (MP = 0.28MJ) object with a radius of 1.11RJ orbiting a G4 star with a period of 4.6 d. WASP-160Bb has a mass and radius (⁠Mp=0.28MJ⁠, Rp=1.09RJ⁠) near-identical to WASP-147b, but is less irradiated, orbiting a metal-rich ([Fe/H]* = 0.27) K0 star with a period of 3.8 d. WASP-160B is part of a near equal-mass visual binary with an on-sky separation of 28.5 arcsec. WASP-164b is a more massive (⁠MP=2.13MJ⁠, Rp=1.13RJ⁠) hot Jupiter, orbiting a G2 star on a close-in (P = 1.8 d), but tidally stable orbit. WASP-165b is a classical (⁠Mp=0.66MJ⁠, RP=1.26RJ⁠) hot Jupiter in a 3.5 d period orbit around a metal-rich ([Fe/H]* = 0.33) star. WASP-147b and WASP-160Bb are promising targets for atmospheric characterization through transmission spectroscopy, while WASP-164b presents a good target for emission spectroscopy.

KW - astro-ph.EP

KW - planets and satellites: detection

KW - planetary systems

UR - https://www.scopus.com/pages/publications/85057146371

U2 - 10.1093/mnras/sty2667

DO - 10.1093/mnras/sty2667

M3 - Article

SN - 0035-8711

VL - 482

SP - 301

EP - 312

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 1

ER -

WASP-147b, 160Bb, 164b and 165b: two hot Saturns and two Jupiters, including two planets with metal-rich hosts

Abstract

Bibliographical note

Keywords

Access to Document

Fingerprint

Cite this