The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab

We present a 0.3−5 μm transmission spectrum of the hot Jupiter HAT-P-32Ab observed with the Space Telescope Imaging Spectrograph and Wide Field Camera 3 instruments mounted on the Hubble Space Telescope, combined with Spitzer Infrared Array Camera photometry. The spectrum is composed of 51 spectroph...

ver descrição completa

Detalhes bibliográficos
Autores: Alam, M. K., López Morales, M., Nikolov, N., Sing, D. K., Henry, G. W., Baxter, C., Désert, J. M., Barstow, J. K., Mikal Evans, T., Bourrier, V., Lavvas, P., Wakeford, H. R., Williamson, M. H., Sanz-Forcada, Jorge, Buchhave, L. A., Cohen, O., García Muñoz, Antonio
Tipo de documento: artigo
Estado:Versão publicada
Data de publicação:2020
País:España
Recursos:Instituto Nacional de Técnica Aeroespacial (INTA)
Repositório:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
OAI Identifier:oai:digital.inta.es:20.500.12666/405
Acesso em linha:https://iopscience.iop.org/article/10.3847/1538-3881/ab96cb
http://hdl.handle.net/20.500.12666/405
https://doi.org/10.3847/1538-3881/ab96cb
Access Level:Acceso aberto
Palavra-chave:Exoplanet atmospheres
Exoplanet atmospheric composition
Exoplanets
Hot Jupiters
id ES_a0e00569f268e8c8e806457ccc21d4fb
oai_identifier_str oai:digital.inta.es:20.500.12666/405
network_acronym_str ES
network_name_str España
repository_id_str
dc.title.none.fl_str_mv The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
title The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
spellingShingle The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
Alam, M. K.
Exoplanet atmospheres
Exoplanet atmospheric composition
Exoplanets
Hot Jupiters
title_short The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
title_full The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
title_fullStr The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
title_full_unstemmed The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
title_sort The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32Ab
dc.creator.none.fl_str_mv Alam, M. K.
López Morales, M.
Nikolov, N.
Sing, D. K.
Henry, G. W.
Baxter, C.
Désert, J. M.
Barstow, J. K.
Mikal Evans, T.
Bourrier, V.
Lavvas, P.
Wakeford, H. R.
Williamson, M. H.
Sanz-Forcada, Jorge
Buchhave, L. A.
Cohen, O.
García Muñoz, Antonio
author Alam, M. K.
author_facet Alam, M. K.
López Morales, M.
Nikolov, N.
Sing, D. K.
Henry, G. W.
Baxter, C.
Désert, J. M.
Barstow, J. K.
Mikal Evans, T.
Bourrier, V.
Lavvas, P.
Wakeford, H. R.
Williamson, M. H.
Sanz-Forcada, Jorge
Buchhave, L. A.
Cohen, O.
García Muñoz, Antonio
author_role author
author2 López Morales, M.
Nikolov, N.
Sing, D. K.
Henry, G. W.
Baxter, C.
Désert, J. M.
Barstow, J. K.
Mikal Evans, T.
Bourrier, V.
Lavvas, P.
Wakeford, H. R.
Williamson, M. H.
Sanz-Forcada, Jorge
Buchhave, L. A.
Cohen, O.
García Muñoz, Antonio
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Alam, M. K. [0000-0003-4157-832X]
López Morales, M. [0000-0003-3204-8183]
Nikolov, N. [0000-0002-6500-3574]
Sing, D. K. [0000-0001-6050-7645]
Henry, G. W. [0000-0003-4155-8513]
Baxter, C. [0000-0003-3438-843X]
Désert, J. M. [0000-0002-0875-8401]
Barstow, J. K. [0000-0003-3726-5419]
Mikal Evans, T. [0000-0001-5442-1300]
Bourrier, V. [0000-0002-9148-034X]
Lavvas, P. [0000-0002-5360-3660]
Wakeford, H. R. [0000-0003-4328-3867]
Forcada, J. S. [0000-0002-1600-7835]
Buchhave, L. A. [0000-0003-1605-5666]
Cohen, O. [0000-0003-3721-0215]
García Muñoz, A. [0000-0003-1756-4825]
Agencia Estatal de Investigación (AEI)
National Aeronautics and Space Administration (NASA)
European Research Council (ERC)
dc.subject.none.fl_str_mv Exoplanet atmospheres
Exoplanet atmospheric composition
Exoplanets
Hot Jupiters
topic Exoplanet atmospheres
Exoplanet atmospheric composition
Exoplanets
Hot Jupiters
description We present a 0.3−5 μm transmission spectrum of the hot Jupiter HAT-P-32Ab observed with the Space Telescope Imaging Spectrograph and Wide Field Camera 3 instruments mounted on the Hubble Space Telescope, combined with Spitzer Infrared Array Camera photometry. The spectrum is composed of 51 spectrophotometric bins with widths ranging between 150 and 400 Å, measured to a median precision of 215 ppm. Comparisons of the observed transmission spectrum to a grid of 1D radiative-convective equilibrium models indicate the presence of clouds/hazes, consistent with previous transit observations and secondary eclipse measurements. To provide more robust constraints on the planet's atmospheric properties, we perform the first full optical to infrared retrieval analysis for this planet. The retrieved spectrum is consistent with a limb temperature of ${1248}_{-92}^{+92}$ K, a thick cloud deck, enhanced Rayleigh scattering, and ~10× solar H2O abundance. We find log(Z/Z⊙) = ${2.41}_{-0.07}^{+0.06}$, and compare this measurement with the mass–metallicity relation derived for the solar system.
publishDate 2020
dc.date.none.fl_str_mv 2020
2021
2021
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv https://iopscience.iop.org/article/10.3847/1538-3881/ab96cb
http://hdl.handle.net/20.500.12666/405
https://doi.org/10.3847/1538-3881/ab96cb
url https://iopscience.iop.org/article/10.3847/1538-3881/ab96cb
http://hdl.handle.net/20.500.12666/405
https://doi.org/10.3847/1538-3881/ab96cb
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv ENANAS MARRONES Y PLANETAS AISLADOS Y COMO COMPAÑEROS DE ESTRELLAS
info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-79425-C3-2-P
Future of upper atmospheric characterisation of exoplanets with spectroscopy
Exploring the Plurality of New Worlds: Their Origins, Climate and Habitability
info:eu-repo/grantAgreement/EC/H2020/679633
info:eu-repo/grantAgreement/EC/H2020/724427
dc.rights.none.fl_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
Published 2020 July 2 • © 2020. The American Astronomical Society. All rights reserved.
https://creativecommons.org/licenses/by-nc-nd/4.0/
info:eu-repo/semantics/openAccess
rights_invalid_str_mv Attribution-NonCommercial-NoDerivatives 4.0 International
Published 2020 July 2 • © 2020. The American Astronomical Society. All rights reserved.
https://creativecommons.org/licenses/by-nc-nd/4.0/
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv application/pdf
dc.publisher.none.fl_str_mv The Institute of Physics (IOP)
publisher.none.fl_str_mv The Institute of Physics (IOP)
dc.source.none.fl_str_mv reponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname:Instituto Nacional de Técnica Aeroespacial (INTA)
instname_str Instituto Nacional de Técnica Aeroespacial (INTA)
reponame_str DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
collection DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
repository.name.fl_str_mv
repository.mail.fl_str_mv
_version_ 1869415064522457088
spelling The Hubble Space Telescope PanCET Program: An Optical to Infrared Transmission Spectrum of HAT-P-32AbAlam, M. K.López Morales, M.Nikolov, N.Sing, D. K.Henry, G. W.Baxter, C.Désert, J. M.Barstow, J. K.Mikal Evans, T.Bourrier, V.Lavvas, P.Wakeford, H. R.Williamson, M. H.Sanz-Forcada, JorgeBuchhave, L. A.Cohen, O.García Muñoz, AntonioExoplanet atmospheresExoplanet atmospheric compositionExoplanetsHot JupitersWe present a 0.3−5 μm transmission spectrum of the hot Jupiter HAT-P-32Ab observed with the Space Telescope Imaging Spectrograph and Wide Field Camera 3 instruments mounted on the Hubble Space Telescope, combined with Spitzer Infrared Array Camera photometry. The spectrum is composed of 51 spectrophotometric bins with widths ranging between 150 and 400 Å, measured to a median precision of 215 ppm. Comparisons of the observed transmission spectrum to a grid of 1D radiative-convective equilibrium models indicate the presence of clouds/hazes, consistent with previous transit observations and secondary eclipse measurements. To provide more robust constraints on the planet's atmospheric properties, we perform the first full optical to infrared retrieval analysis for this planet. The retrieved spectrum is consistent with a limb temperature of ${1248}_{-92}^{+92}$ K, a thick cloud deck, enhanced Rayleigh scattering, and ~10× solar H2O abundance. We find log(Z/Z⊙) = ${2.41}_{-0.07}^{+0.06}$, and compare this measurement with the mass–metallicity relation derived for the solar system.M.K.A. thanks Michael Zhang for useful discussions. This paper makes use of observations from the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with HST GO programs 14767 and 14260. This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. M.K.A. acknowledges support by the National Science Foundation through a Graduate Research Fellowship. V.B. has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation program (project Four Aces; grant agreement No. 724427). J.M.D. acknowledges the European Research Council (ERC) European Unions Horizon 2020 research and innovation program (grant agreement No. 679633; Exo-Atmos) and the Amsterdam Academic Alliance (AAA) Program. G.W.H. acknowledges long-term support from NASA, NSF, Tennessee State University, and the State of Tennessee through its Centers of Excellence Program and from the Space Telescope Science Institute under grant HST-GO-14767. J.S.F. acknnowledges support from the Spanish MINECO through grant AYA2016-79425-C3-2-P. H.R.W. acknowledges support from the Giacconi Prize Fellowship at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc.Peer reviewThe Institute of Physics (IOP)Alam, M. K. [0000-0003-4157-832X]López Morales, M. [0000-0003-3204-8183]Nikolov, N. [0000-0002-6500-3574]Sing, D. K. [0000-0001-6050-7645]Henry, G. W. [0000-0003-4155-8513]Baxter, C. [0000-0003-3438-843X]Désert, J. M. [0000-0002-0875-8401]Barstow, J. K. [0000-0003-3726-5419]Mikal Evans, T. [0000-0001-5442-1300]Bourrier, V. [0000-0002-9148-034X]Lavvas, P. [0000-0002-5360-3660]Wakeford, H. R. [0000-0003-4328-3867]Forcada, J. S. [0000-0002-1600-7835]Buchhave, L. A. [0000-0003-1605-5666]Cohen, O. [0000-0003-3721-0215]García Muñoz, A. [0000-0003-1756-4825]Agencia Estatal de Investigación (AEI)National Aeronautics and Space Administration (NASA)European Research Council (ERC)202120212020info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501application/pdfhttps://iopscience.iop.org/article/10.3847/1538-3881/ab96cbhttp://hdl.handle.net/20.500.12666/405https://doi.org/10.3847/1538-3881/ab96cbreponame:DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacialinstname:Instituto Nacional de Técnica Aeroespacial (INTA)InglésENANAS MARRONES Y PLANETAS AISLADOS Y COMO COMPAÑEROS DE ESTRELLASinfo:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2013-2016/AYA2016-79425-C3-2-PFuture of upper atmospheric characterisation of exoplanets with spectroscopyExploring the Plurality of New Worlds: Their Origins, Climate and Habitabilityinfo:eu-repo/grantAgreement/EC/H2020/679633info:eu-repo/grantAgreement/EC/H2020/724427Attribution-NonCommercial-NoDerivatives 4.0 InternationalPublished 2020 July 2 • © 2020. The American Astronomical Society. All rights reserved.https://creativecommons.org/licenses/by-nc-nd/4.0/info:eu-repo/semantics/openAccessoai:digital.inta.es:20.500.12666/4052026-06-23T12:46:37Z
score 15.228081