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A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey

Schanche, N.; Hébrard, G.; Stassun, K. G.; Hord, B.; Barkaoui, K.; Bieryla, A.; Ciardi, D.; Collins, K. A.; Collier Cameron, A.; Hartman, J.; Heidari, N.; Hellier, C.; Howell, S. B.; Lendl, M.; McCormac, J.; McLeod, K. K.; Parviainen, H.; Radford, D.; Rajpurohit, A. S.; Relles, H.; Sharma, R.; Baliwal, S.; Bakos, G.; Barros, S. C. C.; Bouchy, F.; Burdanov, A.; Budnikova, P. A.; Chakaraborty, A.; Clark, C.; Delrez, Laetitia; Demangeon, O. D. S.; Díaz, R. F.; Donnenfield, J.; Everett, M.; Fukui, A.; Gillon, M.; Hedges, C.; Higuera, J.; Jehin, E.; Jenkins, J. M.; Kiefer, F.; Laloum, D.; Livingston, J.; Lund, M.; Magain, P.; Maxted, P.; Mireles, I.; Murgas, F.; Narita, N.; Nikitha, K. J.; Opitom, C.; Palle, E.; Patel, Y. G.; Rose, M.; Sousa, S. G.; Strakhov, I. A.; Strøm, P.; Tuson, A.; West, R.; Winn, J.

Authors

N. Schanche

G. Hébrard

K. G. Stassun

B. Hord

K. Barkaoui

A. Bieryla

D. Ciardi

K. A. Collins

A. Collier Cameron

J. Hartman

N. Heidari

S. B. Howell

M. Lendl

J. McCormac

K. K. McLeod

H. Parviainen

D. Radford

A. S. Rajpurohit

H. Relles

R. Sharma

S. Baliwal

G. Bakos

S. C. C. Barros

F. Bouchy

A. Burdanov

P. A. Budnikova

A. Chakaraborty

C. Clark

Laetitia Delrez

O. D. S. Demangeon

R. F. Díaz

J. Donnenfield

M. Everett

A. Fukui

M. Gillon

C. Hedges

J. Higuera

E. Jehin

J. M. Jenkins

F. Kiefer

D. Laloum

J. Livingston

M. Lund

P. Magain

I. Mireles

F. Murgas

N. Narita

K. J. Nikitha

C. Opitom

E. Palle

Y. G. Patel

M. Rose

S. G. Sousa

I. A. Strakhov

P. Strøm

A. Tuson

R. West

J. Winn



Abstract

The Wide Angle Search for Planets (WASP) survey provided some of the first transiting hot Jupiter candidates. With the addition of the Transiting Exoplanet Survey Satellite (TESS), many WASP planet candidates have now been revisited and given updated transit parameters. Here, we present nine transiting planets orbiting FGK stars that were identified as candidates by the WASP survey and found to have planetary masses via radial velocity measurements. Subsequent space-based photometry taken by TESS as well as ground-based photometric and spectroscopic measurements have been used to jointly analyze the planetary properties of WASP-102 b, WASP-116 b, WASP-149 b WASP-154 b, WASP-155 b, WASP-188 b, WASP-194 b/HAT-P-71 b, WASP-195 b, and WASP-197 b. These planets have radii between 0.9 RJup and 1.4 RJup, masses between 0.1 MJup and 1.5 MJup, and periods between 1.3 and 6.6 days.

Citation

Schanche, N., Hébrard, G., Stassun, K. G., Hord, B., Barkaoui, K., Bieryla, A., Ciardi, D., Collins, K. A., Collier Cameron, A., Hartman, J., Heidari, N., Hellier, C., Howell, S. B., Lendl, M., McCormac, J., McLeod, K. K., Parviainen, H., Radford, D., Rajpurohit, A. S., Relles, H., …Winn, J. (2025). A Swarm of WASP Planets: Nine Giant Planets Identified by the WASP Survey. Astronomical Journal, 169(6), Article 334. https://doi.org/10.3847/1538-3881/adccc6

Journal Article Type Article
Acceptance Date Apr 7, 2025
Online Publication Date May 27, 2025
Publication Date Jun 2, 2025
Deposit Date Jun 2, 2025
Publicly Available Date Jun 2, 2025
Journal The Astronomical Journal
Print ISSN 0004-6256
Electronic ISSN 1538-3881
Publisher American Astronomical Society
Peer Reviewed Peer Reviewed
Volume 169
Issue 6
Article Number 334
DOI https://doi.org/10.3847/1538-3881/adccc6
Keywords Exoplanet systems, Hot Jupiters, Exoplanets
Public URL https://keele-repository.worktribe.com/output/1243005
Publisher URL https://iopscience.iop.org/article/10.3847/1538-3881/adccc6

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