The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1

We present a 5 Å-100 μm spectral energy distribution (SED) of the ultracool dwarf star TRAPPIST-1, obtained as part of the Mega-MUSCLES Treasury Survey. The SED combines ultraviolet and blue-optical spectroscopy obtained with the Hubble Space Telescope, X-ray spectroscopy obtained with XMM-Newton, a...

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Autores: Wilson, David J., Froning, Cynthia S., Duvvuri, Girish M., France, Kevin, Youngblood, Allison, Schneider, P. Christian, Berta Thompson, Zachory, Brown, Alexander, Buccino, Andrea Paola, Hawley, Suzanne, Irwin, Jonathan, Kaltenegger, Lisa, Kowalski, Adam, Linsky, Jeffrey, Parke Loyd, Robert O., Miguel, Yamila, Pineda, J. Sebastian, Redfield, Seth, Roberge, Aki, Rugheimer, Sarah, Tian, Feng, Vieytes, Mariela Cristina
Tipo de recurso: artículo
Estado:Versión publicada
Fecha de publicación:2021
País:Argentina
Institución:Consejo Nacional de Investigaciones Científicas y Técnicas
Repositorio:CONICET Digital (CONICET)
Idioma:inglés
OAI Identifier:oai:ri.conicet.gov.ar:11336/182451
Acceso en línea:http://hdl.handle.net/11336/182451
Access Level:acceso abierto
Palabra clave:M dwarf stars
Exoplanet astronomy
Exoplanet atmospheres
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
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oai_identifier_str oai:ri.conicet.gov.ar:11336/182451
network_acronym_str AR
network_name_str Argentina
repository_id_str
dc.title.none.fl_str_mv The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
title The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
spellingShingle The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
Wilson, David J.
M dwarf stars
Exoplanet astronomy
Exoplanet atmospheres
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
title_short The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
title_full The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
title_fullStr The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
title_full_unstemmed The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
title_sort The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1
dc.creator.none.fl_str_mv Wilson, David J.
Froning, Cynthia S.
Duvvuri, Girish M.
France, Kevin
Youngblood, Allison
Schneider, P. Christian
Berta Thompson, Zachory
Brown, Alexander
Buccino, Andrea Paola
Hawley, Suzanne
Irwin, Jonathan
Kaltenegger, Lisa
Kowalski, Adam
Linsky, Jeffrey
Parke Loyd, Robert O.
Miguel, Yamila
Pineda, J. Sebastian
Redfield, Seth
Roberge, Aki
Rugheimer, Sarah
Tian, Feng
Vieytes, Mariela Cristina
author Wilson, David J.
author_facet Wilson, David J.
Froning, Cynthia S.
Duvvuri, Girish M.
France, Kevin
Youngblood, Allison
Schneider, P. Christian
Berta Thompson, Zachory
Brown, Alexander
Buccino, Andrea Paola
Hawley, Suzanne
Irwin, Jonathan
Kaltenegger, Lisa
Kowalski, Adam
Linsky, Jeffrey
Parke Loyd, Robert O.
Miguel, Yamila
Pineda, J. Sebastian
Redfield, Seth
Roberge, Aki
Rugheimer, Sarah
Tian, Feng
Vieytes, Mariela Cristina
author_role author
author2 Froning, Cynthia S.
Duvvuri, Girish M.
France, Kevin
Youngblood, Allison
Schneider, P. Christian
Berta Thompson, Zachory
Brown, Alexander
Buccino, Andrea Paola
Hawley, Suzanne
Irwin, Jonathan
Kaltenegger, Lisa
Kowalski, Adam
Linsky, Jeffrey
Parke Loyd, Robert O.
Miguel, Yamila
Pineda, J. Sebastian
Redfield, Seth
Roberge, Aki
Rugheimer, Sarah
Tian, Feng
Vieytes, Mariela Cristina
author2_role 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 M dwarf stars
Exoplanet astronomy
Exoplanet atmospheres
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
topic M dwarf stars
Exoplanet astronomy
Exoplanet atmospheres
https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
description We present a 5 Å-100 μm spectral energy distribution (SED) of the ultracool dwarf star TRAPPIST-1, obtained as part of the Mega-MUSCLES Treasury Survey. The SED combines ultraviolet and blue-optical spectroscopy obtained with the Hubble Space Telescope, X-ray spectroscopy obtained with XMM-Newton, and models of the stellar photosphere, chromosphere, transition region, and corona. A new differential emission measure model of the unobserved extreme-ultraviolet spectrum is provided, improving on the Lyα-EUV relations often used to estimate the 100-911 Å flux from low-mass stars. We describe the observations and models used, as well as the recipe for combining them into an SED. We also provide a semiempirical, noise-free model of the stellar ultraviolet spectrum based on our observations for use in atmospheric modeling of the TRAPPIST-1 planets.
publishDate 2021
dc.date.none.fl_str_mv 2021-04
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/11336/182451
Wilson, David J.; Froning, Cynthia S.; Duvvuri, Girish M.; France, Kevin; Youngblood, Allison; et al.; The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1; IOP Publishing; Astrophysical Journal; 911; 1; 4-2021; 1-16
0004-637X
1538-4357
CONICET Digital
CONICET
url http://hdl.handle.net/11336/182451
identifier_str_mv Wilson, David J.; Froning, Cynthia S.; Duvvuri, Girish M.; France, Kevin; Youngblood, Allison; et al.; The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1; IOP Publishing; Astrophysical Journal; 911; 1; 4-2021; 1-16
0004-637X
1538-4357
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/abe771
info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/abe771
info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2102.11415
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
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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spelling The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1Wilson, David J.Froning, Cynthia S.Duvvuri, Girish M.France, KevinYoungblood, AllisonSchneider, P. ChristianBerta Thompson, ZachoryBrown, AlexanderBuccino, Andrea PaolaHawley, SuzanneIrwin, JonathanKaltenegger, LisaKowalski, AdamLinsky, JeffreyParke Loyd, Robert O.Miguel, YamilaPineda, J. SebastianRedfield, SethRoberge, AkiRugheimer, SarahTian, FengVieytes, Mariela CristinaM dwarf starsExoplanet astronomyExoplanet atmosphereshttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We present a 5 Å-100 μm spectral energy distribution (SED) of the ultracool dwarf star TRAPPIST-1, obtained as part of the Mega-MUSCLES Treasury Survey. The SED combines ultraviolet and blue-optical spectroscopy obtained with the Hubble Space Telescope, X-ray spectroscopy obtained with XMM-Newton, and models of the stellar photosphere, chromosphere, transition region, and corona. A new differential emission measure model of the unobserved extreme-ultraviolet spectrum is provided, improving on the Lyα-EUV relations often used to estimate the 100-911 Å flux from low-mass stars. We describe the observations and models used, as well as the recipe for combining them into an SED. We also provide a semiempirical, noise-free model of the stellar ultraviolet spectrum based on our observations for use in atmospheric modeling of the TRAPPIST-1 planets.Fil: Wilson, David J.. University of Texas at Austin; Estados UnidosFil: Froning, Cynthia S.. University of Texas at Austin; Estados UnidosFil: Duvvuri, Girish M.. State University of Colorado at Boulder; Estados UnidosFil: France, Kevin. State University of Colorado at Boulder; Estados UnidosFil: Youngblood, Allison. Goddard Space Flight Center; Estados Unidos. State University of Colorado at Boulder; Estados UnidosFil: Schneider, P. Christian. Universitat Hamburg; AlemaniaFil: Berta Thompson, Zachory. State University of Colorado at Boulder; Estados UnidosFil: Brown, Alexander. State University of Colorado at Boulder; Estados UnidosFil: Buccino, Andrea Paola. 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. Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Departamento de Física; ArgentinaFil: Hawley, Suzanne. University of Washington; Estados UnidosFil: Irwin, Jonathan. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Kaltenegger, Lisa. Cornell University; Estados UnidosFil: Kowalski, Adam. State University of Colorado at Boulder; Estados UnidosFil: Linsky, Jeffrey. State University of Colorado at Boulder; Estados UnidosFil: Parke Loyd, Robert O.. Arizona State University; Estados UnidosFil: Miguel, Yamila. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Leiden University; Países BajosFil: Pineda, J. Sebastian. State University of Colorado at Boulder; Estados UnidosFil: Redfield, Seth. Ohio Wesleyan University.; Estados UnidosFil: Roberge, Aki. Goddard Space Flight Center; Estados UnidosFil: Rugheimer, Sarah. University of Oxford; Reino UnidoFil: Tian, Feng. Macau University Of Science And Technology; MacaoFil: Vieytes, Mariela Cristina. Consejo Nacional de Investigaciones 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; ArgentinaIOP Publishing2021-04info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/182451Wilson, David J.; Froning, Cynthia S.; Duvvuri, Girish M.; France, Kevin; Youngblood, Allison; et al.; The Mega-MUSCLES Spectral Energy Distribution of TRAPPIST-1; IOP Publishing; Astrophysical Journal; 911; 1; 4-2021; 1-160004-637X1538-4357CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.3847/1538-4357/abe771info:eu-repo/semantics/altIdentifier/url/https://iopscience.iop.org/article/10.3847/1538-4357/abe771info:eu-repo/semantics/altIdentifier/arxiv/https://arxiv.org/abs/2102.11415info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2024-05-08T14:28:51Zoai:ri.conicet.gov.ar:11336/182451instacron: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:34982024-05-08 14:28:51.238CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
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