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

Autores
Hay, K. L.; Collier Cameron, A.; 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.; Diaz, Rodrigo Fernando; Gillon, M.; Gonzàlez, E.; Hellier, C.; Holmes, S.; Jarvis, J. F.; Jehin, E.; Joshi, Y. C.; Kolb, U.; Lendl, M.; Maxted, P. F. L.; Mccormac, J.; Miller, G. R. M.; Mortier, A.; Pollacco, D.; Queloz, D.; Ségransan, D.; Simpson, E. K.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; Vanhuysse, M.; West, R. G.; Wilson, P. A.
Año de publicación
2016
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
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 light curves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 d, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 d 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 = 0.514 ± 0.020MJ and the planet has an orbital period of 4.05 d. They are bright targets (V = 13.18, 10.97 and 11.07, respectively) ideal for further characterization work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. The WASP-93 system has sufficient angular momentum to be tidally migrating outwards if the system is near spin–orbit alignment, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.
Fil: Hay, K. L.. University Of St Andrews; Reino Unido
Fil: Collier Cameron, A.. University Of St Andrews; Reino Unido
Fil: Doyle, A. P.. University Of Warwick; Reino Unido
Fil: Hébrard, G.. Universit´e Pierre & Marie Curie; Francia
Fil: Skillen, I.. Isaac Newton Group of Telescopes; España
Fil: Anderson, D. R.. University, Staffordshire; Reino Unido
Fil: Barros, S. C. C.. Universidad de Porto; Portugal
Fil: Brown, D. J. A.. University Of St Andrews; Reino Unido
Fil: Bouchy, F.. Aix Marseille Universit´e; Francia
Fil: Busuttil, R.. The Open University,; Reino Unido
Fil: Delorme, P.. University Of St Andrews; Reino Unido
Fil: Delrez, L.. Universite de Liege; Bélgica
Fil: Demangeon, O.. Aix Marseille Universite; Francia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Gillon, M.. Universite de Liege; Bélgica
Fil: Gonzàlez, E.. Observatori Astron´omic de Mallorca; España
Fil: Hellier, C.. Keele University; Reino Unido
Fil: Holmes, S.. The Open University; Reino Unido
Fil: Jarvis, J. F.. The Open University; Reino Unido
Fil: Jehin, E.. Aix Marseille Universit´e; Francia
Fil: Joshi, Y. C.. Queen’s University; Reino Unido
Fil: Kolb, U.. The Open University; Reino Unido
Fil: Lendl, M.. Observatoire de Geneve; Suiza
Fil: Maxted, P. F. L.. Keele University, Staffordshire; Reino Unido
Fil: Mccormac, J.. University Of Warwick; Reino Unido
Fil: Miller, G. R. M.. University Of St Andrews; Reino Unido
Fil: Mortier, A.. University Of St Andrews; Reino Unido
Fil: Pollacco, D.. University Of Warwick; Reino Unido
Fil: Queloz, D.. University of Cambridge; Reino Unido
Fil: Ségransan, D.. Observatoire de Geneve; Suiza
Fil: Simpson, E. K.. Queen’s University,; Reino Unido
Fil: Smalley, B.. Keele University; Reino Unido
Fil: Southworth, J.. Keele University; Reino Unido
Fil: Triaud, A. H. M. J.. University of Cambridge; Reino Unido
Fil: Turner, O. D.. Keele University; Reino Unido
Fil: Udry, S.. bservatoire de Geneve; Suiza
Fil: Vanhuysse, M.. OverSky,; Francia
Fil: West, R. G.. University Of Warwick; Reino Unido
Fil: Wilson, P. A.. Institut d’Astrophysique de Paris; Francia
Materia
techniques: photometric
techniques: radial velocities
planets and satellites: detection
planet-star interactions
planetary systems
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/18435

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oai_identifier_str oai:ri.conicet.gov.ar:11336/18435
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planetsHay, K. L.Collier Cameron, A.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.Diaz, Rodrigo FernandoGillon, M.Gonzàlez, E.Hellier, C.Holmes, S.Jarvis, J. F.Jehin, E.Joshi, Y. C.Kolb, U.Lendl, M.Maxted, P. F. L.Mccormac, J.Miller, G. R. M.Mortier, A.Pollacco, D.Queloz, D.Ségransan, D.Simpson, E. K.Smalley, B.Southworth, J.Triaud, A. H. M. J.Turner, O. D.Udry, S.Vanhuysse, M.West, R. G.Wilson, P. A.techniques: photometrictechniques: radial velocitiesplanets and satellites: detectionplanet-star interactionsplanetary systemshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We 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 light curves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 d, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 d 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 = 0.514 ± 0.020MJ and the planet has an orbital period of 4.05 d. They are bright targets (V = 13.18, 10.97 and 11.07, respectively) ideal for further characterization work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. The WASP-93 system has sufficient angular momentum to be tidally migrating outwards if the system is near spin–orbit alignment, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.Fil: Hay, K. L.. University Of St Andrews; Reino UnidoFil: Collier Cameron, A.. University Of St Andrews; Reino UnidoFil: Doyle, A. P.. University Of Warwick; Reino UnidoFil: Hébrard, G.. Universit´e Pierre & Marie Curie; FranciaFil: Skillen, I.. Isaac Newton Group of Telescopes; EspañaFil: Anderson, D. R.. University, Staffordshire; Reino UnidoFil: Barros, S. C. C.. Universidad de Porto; PortugalFil: Brown, D. J. A.. University Of St Andrews; Reino UnidoFil: Bouchy, F.. Aix Marseille Universit´e; FranciaFil: Busuttil, R.. The Open University,; Reino UnidoFil: Delorme, P.. University Of St Andrews; Reino UnidoFil: Delrez, L.. Universite de Liege; BélgicaFil: Demangeon, O.. Aix Marseille Universite; FranciaFil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Gillon, M.. Universite de Liege; BélgicaFil: Gonzàlez, E.. Observatori Astron´omic de Mallorca; EspañaFil: Hellier, C.. Keele University; Reino UnidoFil: Holmes, S.. The Open University; Reino UnidoFil: Jarvis, J. F.. The Open University; Reino UnidoFil: Jehin, E.. Aix Marseille Universit´e; FranciaFil: Joshi, Y. C.. Queen’s University; Reino UnidoFil: Kolb, U.. The Open University; Reino UnidoFil: Lendl, M.. Observatoire de Geneve; SuizaFil: Maxted, P. F. L.. Keele University, Staffordshire; Reino UnidoFil: Mccormac, J.. University Of Warwick; Reino UnidoFil: Miller, G. R. M.. University Of St Andrews; Reino UnidoFil: Mortier, A.. University Of St Andrews; Reino UnidoFil: Pollacco, D.. University Of Warwick; Reino UnidoFil: Queloz, D.. University of Cambridge; Reino UnidoFil: Ségransan, D.. Observatoire de Geneve; SuizaFil: Simpson, E. K.. Queen’s University,; Reino UnidoFil: Smalley, B.. Keele University; Reino UnidoFil: Southworth, J.. Keele University; Reino UnidoFil: Triaud, A. H. M. J.. University of Cambridge; Reino UnidoFil: Turner, O. D.. Keele University; Reino UnidoFil: Udry, S.. bservatoire de Geneve; SuizaFil: Vanhuysse, M.. OverSky,; FranciaFil: West, R. G.. University Of Warwick; Reino UnidoFil: Wilson, P. A.. Institut d’Astrophysique de Paris; FranciaOxford University Press2016-08-20info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/18435Hay, K. L.; Collier Cameron, A.; Doyle, A. P.; Hébrard, G.; Skillen, I.; et al.; WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 463; 3; 20-8-2016; 3276-32890035-8711CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw2090info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1607.00774info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/463/3/3276/2646547/WASP-92b-WASP-93b-and-WASP-118b-three-new?cited-by=yes&legid=mnras;463/3/3276info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:33:19Zoai:ri.conicet.gov.ar:11336/18435instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:33:19.804CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
title WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
spellingShingle WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
Hay, K. L.
techniques: photometric
techniques: radial velocities
planets and satellites: detection
planet-star interactions
planetary systems
title_short WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
title_full WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
title_fullStr WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
title_full_unstemmed WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
title_sort WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets
dc.creator.none.fl_str_mv Hay, K. L.
Collier Cameron, A.
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.
Diaz, Rodrigo Fernando
Gillon, M.
Gonzàlez, E.
Hellier, C.
Holmes, S.
Jarvis, J. F.
Jehin, E.
Joshi, Y. C.
Kolb, U.
Lendl, M.
Maxted, P. F. L.
Mccormac, J.
Miller, G. R. M.
Mortier, A.
Pollacco, D.
Queloz, D.
Ségransan, D.
Simpson, E. K.
Smalley, B.
Southworth, J.
Triaud, A. H. M. J.
Turner, O. D.
Udry, S.
Vanhuysse, M.
West, R. G.
Wilson, P. A.
author Hay, K. L.
author_facet Hay, K. L.
Collier Cameron, A.
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.
Diaz, Rodrigo Fernando
Gillon, M.
Gonzàlez, E.
Hellier, C.
Holmes, S.
Jarvis, J. F.
Jehin, E.
Joshi, Y. C.
Kolb, U.
Lendl, M.
Maxted, P. F. L.
Mccormac, J.
Miller, G. R. M.
Mortier, A.
Pollacco, D.
Queloz, D.
Ségransan, D.
Simpson, E. K.
Smalley, B.
Southworth, J.
Triaud, A. H. M. J.
Turner, O. D.
Udry, S.
Vanhuysse, M.
West, R. G.
Wilson, P. A.
author_role author
author2 Collier Cameron, A.
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.
Diaz, Rodrigo Fernando
Gillon, M.
Gonzàlez, E.
Hellier, C.
Holmes, S.
Jarvis, J. F.
Jehin, E.
Joshi, Y. C.
Kolb, U.
Lendl, M.
Maxted, P. F. L.
Mccormac, J.
Miller, G. R. M.
Mortier, A.
Pollacco, D.
Queloz, D.
Ségransan, D.
Simpson, E. K.
Smalley, B.
Southworth, J.
Triaud, A. H. M. J.
Turner, O. D.
Udry, S.
Vanhuysse, M.
West, R. G.
Wilson, P. A.
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv techniques: photometric
techniques: radial velocities
planets and satellites: detection
planet-star interactions
planetary systems
topic techniques: photometric
techniques: radial velocities
planets and satellites: detection
planet-star interactions
planetary systems
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv 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 light curves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 d, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 d 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 = 0.514 ± 0.020MJ and the planet has an orbital period of 4.05 d. They are bright targets (V = 13.18, 10.97 and 11.07, respectively) ideal for further characterization work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. The WASP-93 system has sufficient angular momentum to be tidally migrating outwards if the system is near spin–orbit alignment, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.
Fil: Hay, K. L.. University Of St Andrews; Reino Unido
Fil: Collier Cameron, A.. University Of St Andrews; Reino Unido
Fil: Doyle, A. P.. University Of Warwick; Reino Unido
Fil: Hébrard, G.. Universit´e Pierre & Marie Curie; Francia
Fil: Skillen, I.. Isaac Newton Group of Telescopes; España
Fil: Anderson, D. R.. University, Staffordshire; Reino Unido
Fil: Barros, S. C. C.. Universidad de Porto; Portugal
Fil: Brown, D. J. A.. University Of St Andrews; Reino Unido
Fil: Bouchy, F.. Aix Marseille Universit´e; Francia
Fil: Busuttil, R.. The Open University,; Reino Unido
Fil: Delorme, P.. University Of St Andrews; Reino Unido
Fil: Delrez, L.. Universite de Liege; Bélgica
Fil: Demangeon, O.. Aix Marseille Universite; Francia
Fil: Diaz, Rodrigo Fernando. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Gillon, M.. Universite de Liege; Bélgica
Fil: Gonzàlez, E.. Observatori Astron´omic de Mallorca; España
Fil: Hellier, C.. Keele University; Reino Unido
Fil: Holmes, S.. The Open University; Reino Unido
Fil: Jarvis, J. F.. The Open University; Reino Unido
Fil: Jehin, E.. Aix Marseille Universit´e; Francia
Fil: Joshi, Y. C.. Queen’s University; Reino Unido
Fil: Kolb, U.. The Open University; Reino Unido
Fil: Lendl, M.. Observatoire de Geneve; Suiza
Fil: Maxted, P. F. L.. Keele University, Staffordshire; Reino Unido
Fil: Mccormac, J.. University Of Warwick; Reino Unido
Fil: Miller, G. R. M.. University Of St Andrews; Reino Unido
Fil: Mortier, A.. University Of St Andrews; Reino Unido
Fil: Pollacco, D.. University Of Warwick; Reino Unido
Fil: Queloz, D.. University of Cambridge; Reino Unido
Fil: Ségransan, D.. Observatoire de Geneve; Suiza
Fil: Simpson, E. K.. Queen’s University,; Reino Unido
Fil: Smalley, B.. Keele University; Reino Unido
Fil: Southworth, J.. Keele University; Reino Unido
Fil: Triaud, A. H. M. J.. University of Cambridge; Reino Unido
Fil: Turner, O. D.. Keele University; Reino Unido
Fil: Udry, S.. bservatoire de Geneve; Suiza
Fil: Vanhuysse, M.. OverSky,; Francia
Fil: West, R. G.. University Of Warwick; Reino Unido
Fil: Wilson, P. A.. Institut d’Astrophysique de Paris; Francia
description 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 light curves. WASP-92 is an F7 star, with a moderately inflated planet orbiting with a period of 2.17 d, which has Rp = 1.461 ± 0.077RJ and Mp = 0.805 ± 0.068MJ. WASP-93b orbits its F4 host star every 2.73 d 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 = 0.514 ± 0.020MJ and the planet has an orbital period of 4.05 d. They are bright targets (V = 13.18, 10.97 and 11.07, respectively) ideal for further characterization work, particularly WASP-118b, which is being observed by K2 as part of campaign 8. The WASP-93 system has sufficient angular momentum to be tidally migrating outwards if the system is near spin–orbit alignment, which is divergent from the tidal behaviour of the majority of hot Jupiters discovered.
publishDate 2016
dc.date.none.fl_str_mv 2016-08-20
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/18435
Hay, K. L.; Collier Cameron, A.; Doyle, A. P.; Hébrard, G.; Skillen, I.; et al.; WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 463; 3; 20-8-2016; 3276-3289
0035-8711
CONICET Digital
CONICET
url http://hdl.handle.net/11336/18435
identifier_str_mv Hay, K. L.; Collier Cameron, A.; Doyle, A. P.; Hébrard, G.; Skillen, I.; et al.; WASP-92b, WASP-93b and WASP-118b: three new transiting close-in giant planets; Oxford University Press; Monthly Notices Of The Royal Astronomical Society; 463; 3; 20-8-2016; 3276-3289
0035-8711
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.1093/mnras/stw2090
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1607.00774
info:eu-repo/semantics/altIdentifier/url/https://academic.oup.com/mnras/article-abstract/463/3/3276/2646547/WASP-92b-WASP-93b-and-WASP-118b-three-new?cited-by=yes&legid=mnras;463/3/3276
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv Oxford University Press
publisher.none.fl_str_mv Oxford University Press
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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