_version_ 1866913788518727680
author Schanche, Nicole
Hébrard, Guillaume
Stassun, Keivan G.
Hord, Benjamin J.
Barkaoui, Khalid
Bieryla, Allyson
Ciardi, David R.
Collins, Karen A.
Cameron, Andrew Collier
Hartman, Joel
Heidari, N.
Hellier, Coel
Howell, Steve B.
Lendl, Monika
McCormac, James
McLeod, Kim K.
Parviainen, Hannu
Radford, Don J.
Rajpurohit, Arvind Singh
Relles, Howard M.
Sharma, Rishikesh
Baliwal, Sanjay
Bakos, Gaspar
Barros, Susana
Bouchy, François
Burdanov, Artem Y.
Budnikova, Polina A.
Chakaraborty, Abhijit
Clark, Catherine
Delrez, Laetitia
Demangeon, O. D. S.
Diaz, Rodrigo
Donnenfield, Jonah
Everett, Mark
Gillon, Michaël
Hedges, Christina
Higuera, Jesus
Jehin, Emmanuel
Jenkins, Jon M.
Kiefer, Flavien
Laloum, Didier
Lund, Mike
Magain, Pierre
Maxted, Pierre
Mireles, Ismael
Nikitha, K. J.
Opitom, Cyrielle
Patel, Yatrik
Rose, Mark
Sousa, Sergio
Strakhov, Ivan
Strøm, Paul
Tuson, Amy
West, Richard
Winn, Joshua
author_facet Schanche, Nicole
Hébrard, Guillaume
Stassun, Keivan G.
Hord, Benjamin J.
Barkaoui, Khalid
Bieryla, Allyson
Ciardi, David R.
Collins, Karen A.
Cameron, Andrew Collier
Hartman, Joel
Heidari, N.
Hellier, Coel
Howell, Steve B.
Lendl, Monika
McCormac, James
McLeod, Kim K.
Parviainen, Hannu
Radford, Don J.
Rajpurohit, Arvind Singh
Relles, Howard M.
Sharma, Rishikesh
Baliwal, Sanjay
Bakos, Gaspar
Barros, Susana
Bouchy, François
Burdanov, Artem Y.
Budnikova, Polina A.
Chakaraborty, Abhijit
Clark, Catherine
Delrez, Laetitia
Demangeon, O. D. S.
Diaz, Rodrigo
Donnenfield, Jonah
Everett, Mark
Gillon, Michaël
Hedges, Christina
Higuera, Jesus
Jehin, Emmanuel
Jenkins, Jon M.
Kiefer, Flavien
Laloum, Didier
Lund, Mike
Magain, Pierre
Maxted, Pierre
Mireles, Ismael
Nikitha, K. J.
Opitom, Cyrielle
Patel, Yatrik
Rose, Mark
Sousa, Sergio
Strakhov, Ivan
Strøm, Paul
Tuson, Amy
West, Richard
Winn, Joshua
contents 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 9 transiting planets orbiting FGK stars that were identified as candidates by the WASP survey and measured to have planetary masses by 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 R_Jup and 1.4 R_Jup, masses between 0.1 M_Jup and 1.5 M_Jup, and periods between 1.3 and 6.6 days.
format Preprint
id arxiv_https___arxiv_org_abs_2504_08091
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle A Swarm of WASP Planets: Nine giant planets identified by the WASP survey
Schanche, Nicole
Hébrard, Guillaume
Stassun, Keivan G.
Hord, Benjamin J.
Barkaoui, Khalid
Bieryla, Allyson
Ciardi, David R.
Collins, Karen A.
Cameron, Andrew Collier
Hartman, Joel
Heidari, N.
Hellier, Coel
Howell, Steve B.
Lendl, Monika
McCormac, James
McLeod, Kim K.
Parviainen, Hannu
Radford, Don J.
Rajpurohit, Arvind Singh
Relles, Howard M.
Sharma, Rishikesh
Baliwal, Sanjay
Bakos, Gaspar
Barros, Susana
Bouchy, François
Burdanov, Artem Y.
Budnikova, Polina A.
Chakaraborty, Abhijit
Clark, Catherine
Delrez, Laetitia
Demangeon, O. D. S.
Diaz, Rodrigo
Donnenfield, Jonah
Everett, Mark
Gillon, Michaël
Hedges, Christina
Higuera, Jesus
Jehin, Emmanuel
Jenkins, Jon M.
Kiefer, Flavien
Laloum, Didier
Lund, Mike
Magain, Pierre
Maxted, Pierre
Mireles, Ismael
Nikitha, K. J.
Opitom, Cyrielle
Patel, Yatrik
Rose, Mark
Sousa, Sergio
Strakhov, Ivan
Strøm, Paul
Tuson, Amy
West, Richard
Winn, Joshua
Earth and Planetary Astrophysics
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 9 transiting planets orbiting FGK stars that were identified as candidates by the WASP survey and measured to have planetary masses by 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 R_Jup and 1.4 R_Jup, masses between 0.1 M_Jup and 1.5 M_Jup, and periods between 1.3 and 6.6 days.
title A Swarm of WASP Planets: Nine giant planets identified by the WASP survey
topic Earth and Planetary Astrophysics
url https://arxiv.org/abs/2504.08091