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
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/18435
Ver los metadatos del registro completo
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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 Técnicas2025-10-22T12:05:54Zoai: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:34982025-10-22 12:05:55.002CONICET 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 |
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info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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openAccess |
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https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
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application/pdf application/pdf |
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Oxford University Press |
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Oxford University Press |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar |
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