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TOI-663: A newly discovered multi-planet system with three transiting mini-Neptunes orbiting an early M star
Indexado
WoS WOS:001231008100005
Scopus SCOPUS_ID:85192824547
DOI 10.1051/0004-6361/202346899
Año 2024
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



We present the detection of three exoplanets orbiting the early M dwarf TOI-663 (TIC 54962195; V = 13.7 mag, J = 10.4 mag, R-star = 0.512 +/- 0.015 R-circle dot, M-star = 0.514 +/- 0.012 M-circle dot, d = 64 pc). TOI-663 b, c, and d, with respective radii of 2.27 +/- 0.10 R-circle plus, 2.26 +/- 0.10 R-circle plus, and 1.92 +/- 0.13 R-circle plus and masses of 4.45 +/- 0.65 M-circle plus, 3.65 +/- 0.97 M-circle plus, and <5.2 M-circle plus at 99%, are located just above the radius valley that separates rocky and volatile-rich exoplanets. The planet candidates are identified in two TESS sectors and are validated with ground-based photometric follow-up, precise radial-velocity measurements, and high-resolution imaging. We used the software package juliet to jointly model the photometric and radial-velocity datasets, with Gaussian processes applied to correct for systematics. The three planets discovered in the TOI-663 system are low-mass mini-Neptunes with radii significantly larger than those of rocky analogs, implying that volatiles, such as water, must predominate. In addition to this internal structure analysis, we also performed a dynamical analysis that confirmed the stability of the system. The three exoplanets in the TOI-663 system, similarly to other sub-Neptunes orbiting M dwarfs, have been found to have lower densities than planets of similar sizes orbiting stars of different spectral types.

Revista



Revista ISSN
Astronomy & Astrophysics 0004-6361

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Disciplinas de Investigación



WOS
Astronomy & Astrophysics
Scopus
Sin Disciplinas
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Cointepas, Marion Mujer Univ Grenoble Alpes - Francia
Univ Geneva - Suiza
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) - Francia
Faculty of Science - Suiza
2 Bouchy, Francois Hombre Univ Geneva - Suiza
Faculty of Science - Suiza
3 Almenara, Jose-Manuel Hombre Univ Grenoble Alpes - Francia
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) - Francia
4 Bonfils, Xavier Hombre Univ Grenoble Alpes - Francia
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) - Francia
5 Astudillo-Defru, Nicola Mujer Universidad Católica de la Santísima Concepción - Chile
6 Knierim, H. - UNIV ZURICH - Suiza
Universität Zürich - Suiza
7 Stalport, M. Hombre Univ Liege - Bélgica
Universite de Liege - Bélgica
MIT - Estados Unidos
MIT Kavli Institute for Astrophysics and Space Research - Estados Unidos
Massachusetts Institute of Technology - Estados Unidos
MIT School of Engineering - Estados Unidos
8 Mignon, Lucille Mujer Univ Geneva - Suiza
Faculty of Science - Suiza
9 Grieves, Nolan Hombre Univ Geneva - Suiza
Faculty of Science - Suiza
10 Bean, Jacob L. Hombre UNIV CHICAGO - Estados Unidos
The Department of Astronomy and Astrophysics, The University of Chicago - Estados Unidos
11 Brady, M. Mujer UNIV CHICAGO - Estados Unidos
The Department of Astronomy and Astrophysics, The University of Chicago - Estados Unidos
12 Burt, Jennifer A. Mujer CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos
13 Martins, B. L. Canto Hombre Univ Fed Rio Grande do Norte - Brasil
Universidade Federal do Rio Grande do Norte - Brasil
14 Pearce, Logan Hombre Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
George Mason Univ - Estados Unidos
George Mason University - Estados Unidos
15 Pearce, Logan Hombre Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
George Mason Univ - Estados Unidos
George Mason University - Estados Unidos
16 Delfosse, Xavier Hombre Univ Grenoble Alpes - Francia
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) - Francia
17 de Medeiros, Jose R. Hombre Univ Fed Rio Grande do Norte - Brasil
Universidade Federal do Rio Grande do Norte - Brasil
18 Demory, Brice-Olivier - Univ Bern - Suiza
University of Bern - Suiza
19 Dorn, C. Mujer Swiss Fed Inst Technol - Suiza
ETH Zurich - Suiza
20 Forveille, Thierry Hombre Univ Grenoble Alpes - Francia
Institut de Planétologie et d’Astrophysique de Grenoble (IPAG) - Francia
21 Fukui, Akihiko Hombre IAC - España
Univ Tokyo - Japón
Instituto Astrofisico de Canarias - España
The University of Tokyo - Japón
22 Gan, Tianjun - Tsinghua Univ - China
Tsinghua University - China
23 Gomez Maqueo Chew, Y. - Universidad Nacional Autónoma de México - México
23 Chew, Y. Gomez Maqueo - Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México
24 Halverson, Sam Hombre CALTECH - Estados Unidos
California Institute of Technology - Estados Unidos
25 Helled, Ravit Mujer UNIV ZURICH - Suiza
Universität Zürich - Suiza
26 Helm, I. - George Mason Univ - Estados Unidos
George Mason University - Estados Unidos
27 Hirano, Teruyuki - Astrobiol Ctr - Japón
Natl Astron Observ Japan - Japón
National Institutes of Natural Sciences - AstroBiology Center - Japón
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón
28 Horne, Keith Hombre Univ St Andrews - Reino Unido
University of St Andrews - Reino Unido
29 Howell, S. Hombre NASA - Estados Unidos
NASA Ames Research Center - Estados Unidos
30 Isogai, Keisuke I. Hombre KYOTO UNIV - Japón
Univ Tokyo - Japón
Kyoto University - Japón
The University of Tokyo - Japón
31 Kasper, David Hombre UNIV CHICAGO - Estados Unidos
The Department of Astronomy and Astrophysics, The University of Chicago - Estados Unidos
32 Kawauchi, K. - Univ Tokyo - Japón
Ritsumeikan Univ - Japón
The University of Tokyo - Japón
Ritsumeikan University Biwako-Kusatsu Campus - Japón
33 Livingston, J. H. Hombre Astrobiol Ctr - Japón
Natl Astron Observ Japan - Japón
Grad Univ Adv Studies - Japón
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón
National Institutes of Natural Sciences - AstroBiology Center - Japón
The Graduate University for Advanced Studies - Japón
34 Massey, Robert Hombre Villa 39 Observ - Estados Unidos
Villa’39 Observatory - Estados Unidos
35 Matson, Rachel A. Mujer US Naval Observ - Estados Unidos
U.S. Naval Observatory - Estados Unidos
36 Murgas, Felipe Hombre IAC - España
ULL - España
Instituto Astrofisico de Canarias - España
Universidad de La Laguna - España
37 Narita, Norio Hombre IAC - España
Univ Tokyo - Japón
Astrobiol Ctr - Japón
Instituto Astrofisico de Canarias - España
The University of Tokyo - Japón
National Institutes of Natural Sciences - AstroBiology Center - Japón
38 Palle, Enric Hombre IAC - España
ULL - España
Instituto Astrofisico de Canarias - España
Universidad de La Laguna - España
39 Relles, Howard M. Hombre Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
40 Sabin, Laurence Mujer Univ Nacl Autonoma Mexico - México
Universidad Nacional Autónoma de México - México
41 Schanche, N. Mujer UNIV MARYLAND - Estados Unidos
University of Maryland, College Park - Estados Unidos
42 Schwarz, Richard P. Hombre Harvard & Smithsonian - Estados Unidos
Harvard-Smithsonian Center for Astrophysics - Estados Unidos
43 Seifahrt, Andreas Hombre UNIV CHICAGO - Estados Unidos
The Department of Astronomy and Astrophysics, The University of Chicago - Estados Unidos
44 Shporer, Avi - MIT - Estados Unidos
MIT Kavli Institute for Astrophysics and Space Research - Estados Unidos
Massachusetts Institute of Technology - Estados Unidos
45 Stefansson, Gudmundur - Princeton Univ - Estados Unidos
Princeton University - Estados Unidos
46 Stuermer, J. Hombre Heidelberg Univ - Alemania
Landessternwarte Heidelberg - Alemania
47 Tamura, Motohide - Astrobiol Ctr - Japón
Natl Astron Observ Japan - Japón
Univ Tokyo - Japón
National Institutes of Natural Sciences - AstroBiology Center - Japón
National Institutes of Natural Sciences - National Astronomical Observatory of Japan - Japón
The University of Tokyo - Japón
48 Tan, T. -G. - Perth Exoplanet Survey Telescope - Australia
49 Twicken, Joseph D. Hombre NASA - Estados Unidos
SETI Inst - Estados Unidos
NASA Ames Research Center - Estados Unidos
SETI Institute - Estados Unidos
50 Watanabe, Noriharu - Univ Tokyo - Japón
The University of Tokyo - Japón
51 Wells, R. D. - Univ Bern - Suiza
University of Bern - Suiza
52 Wilkin, F. P. - Union Coll - Estados Unidos
Union College, Schenectady - Estados Unidos
53 Ricker, George R. Hombre MIT - Estados Unidos
MIT Kavli Institute for Astrophysics and Space Research - Estados Unidos
Massachusetts Institute of Technology - Estados Unidos
54 Stalport, M. Hombre Univ Liege - Bélgica
Universite de Liege - Bélgica
MIT - Estados Unidos
MIT Kavli Institute for Astrophysics and Space Research - Estados Unidos
Massachusetts Institute of Technology - Estados Unidos
MIT School of Engineering - Estados Unidos
55 Winn, J. N. - Princeton Univ - Estados Unidos
Princeton University - Estados Unidos
56 JENKINS, JAMES STEWART Hombre NASA - Estados Unidos
NASA Ames Research Center - Estados Unidos

Muestra la afiliación y género (detectado) para los co-autores de la publicación.

Financiamiento



Fuente
CAPES
National Science Foundation
CNPq
Conselho Nacional de Desenvolvimento Científico e Tecnológico
Coordenação de Aperfeiçoamento de Pessoal de Nível Superior
Universidad Nacional Autónoma de México
NSF
UNAM
University of Bern
JSPS KAKENHI
European Research Council
National Aeronautics and Space Administration (NASA)
NASA
Japan Science and Technology Agency
Japan Society for the Promotion of Science
Swiss National Science Foundation
Swiss National Science Foundation (SNSF)
National Aeronautics and Space Administration
Instituto de Astrofisica de Canarias
NASA Explorer Program
Ames Research Center
Gemini Observatory
Space Telescope Science Institute
Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung
Korea Astronomy and Space Science Institute
NASA's Science Mission directorate
California Institute of Technology
LCOGT network
National Research Council Canada
National Science Foundation Graduate Research Fellowship
Geneva University
NASA Exoplanet Exploration Program
European Research Council under the ERC
NASA through the NASA Hubble Fellowship
Korea Astronomy and Space Science Institute (Republic of Korea)
NASA High-End Computing (HEC) Program through the NASA
Ministério da Ciência, Tecnologia, Inovações e Comunicações
Ministry of Science, ICT and Future Planning
National Research Council (Canada)
JST CREST
Agencia Nacional de Investigación y Desarrollo
Baja California, México
Agencia Nacional de Investigacion y Desarrollo (Chile)
NOIRLab
Science Mission Directorate
Astrobiology Center
National Centre for Competence in Research
Ministerio de Ciencia, Tecnología e Innovación
Ministerio da Ciencia, Tecnologia, Inovacoes e Comunicacoes (Brazil)
NOIRLab through the Mid-Scale Innovations Program (MSIP) - NSF
Amsterdam Brain and Cognition
National Centre for Competence in Research PlanetS
Centre for Space and Habitability
Sierra de San Pedro Mártir
Centre for Space and Habitability (CSH) of the University of Bern
Maunakea Science Reserve and adjacent to the summit of Maunakea
National Centre for Competence in Research 'PlanetS'

Muestra la fuente de financiamiento declarada en la publicación.

Agradecimientos



Agradecimiento
26134/ExoFOP5) website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Funding for the TESS mission is provided by NASA's Science Mission Directorate. This work is partly supported by JSPS KAKENHI Grant Numbers JP17H04574, JP18H05439, JP 18H05442, JP19K14783, JP20K14521, JP21H00035, JP21K13955, JP21K20376, Grant-in-Aid for JSPS Fellows, Grant Number JP20J21872, JST CREST Grant Number JPMJCR1761, and Astrobiology Center SATELLITE Research project AB022006. This article is based on observations made with the MuSCAT2 instrument, developed by ABC, at Telescopio Carlos Sanchez operated on the island of Tenerife by the IAC in the Spanish Observatorio del Teide. M.T. is supported by JSPS KAKENHI grant Nos.18H05442. C.D. acknowledges support from the Swiss National Science Foundation under grant TMSGI2_211313. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE 1746045. G.S. acknowledges support provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51519.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. J.R.M. and B.L.C.M. acknowledge continuous grants from the brazilian funding agencies CAPES (Finance Code 001) and CNPq. The material is based upon work supported by NASA under award number 80GSFC21M0002.
26134/ExoFOP5) website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Funding for the TESS mission is provided by NASA's Science Mission Directorate. This work is partly supported by JSPS KAKENHI Grant Numbers JP17H04574, JP18H05439, JP 18H05442, JP19K14783, JP20K14521, JP21H00035, JP21K13955, JP21K20376, Grant-in-Aid for JSPS Fellows, Grant Number JP20J21872, JST CREST Grant Number JPMJCR1761, and Astrobiology Center SATELLITE Research project AB022006. This article is based on observations made with the MuSCAT2 instrument, developed by ABC, at Telescopio Carlos Sanchez operated on the island of Tenerife by the IAC in the Spanish Observatorio del Teide. M.T. is supported by JSPS KAKENHI grant Nos.18H05442. C.D. acknowledges support from the Swiss National Science Foundation under grant TMSGI2_211313. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE 1746045. G.S. acknowledges support provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51519.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. J.R.M. and B.L.C.M. acknowledge continuous grants from the brazilian funding agencies CAPES (Finance Code 001) and CNPq. The material is based upon work supported by NASA under award number 80GSFC21M0002.
We are grateful to the ESO/La Silla staff for their continuous support. We acknowledge funding from the European Research Council under the ERC Grant Agreement n. 337591-ExTrA. This paper includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA Explorer Program. We acknowledge the use of public TESS Alert data from the pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. Resources supporting this work were provided by the NASA High-End Computing (HEC) program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. We thank the Swiss National Science Foundation (SNSF) and the Geneva University for their continuous support to our planet search programs. This work has been in particular carried out in the frame of the National Centre for Competence in Research \u2018PlanetS\u2019 supported by the Swiss National Science Foundation (SNSF). This work made use of tpfplotter by J. Lillo-Box (publicly available in www.github.com/jlillo/tpfplotter), which also made use of the python packages astropy, lightkurve, matplotlib and numpy. This research was carried out in part at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). Some of the observations in this paper made use of the High-Resolution Imaging instrument Zorro and were obtained under Gemini LLP Proposal Number: GN/S-2021A-LP-105. Zorro was funded by the NASA Exoplanet Exploration Program and built at the NASA Ames Research Center by Steve B. Howell, Nic Scott, Elliott P. Horch, and Emmett Quigley. Zorro was mounted on the Gemini South telescope of the international Gemini Observatory, a program of NSF\u2019s OIR Lab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation on behalf of the Gemini partnership: the National Science Foundation (United States), National Research Council (Canada), Agencia Nacional de Investigaci\u00F3n y Desarrollo (Chile), Ministerio de Ciencia, Tecnolog\u00EDa e Innovaci\u00F3n (Argentina), Minist\u00E9rio da Ci\u00EAncia, Tecnologia, Inova\u00E7\u00F5es e Comunica\u00E7\u00F5es (Brazil), and Korea Astronomy and Space Science Institute (Republic of Korea). Some observations in this paper were obtained with MAROON-X, a visitor instrument on the Gemini North telescope, located within the Maunakea Science Reserve and adjacent to the summit of Maunakea. We are grateful for the privilege of observing the Universe from a place that is unique in both its astronomical quality and its cultural significance. This work is based upon observations carried out at the Observatorio Astron\u00F3mico Nacional on the Sierra de San Pedro M\u00E1rtir (OAN-SPM), Baja California, M\u00E9xico. SAINT-EX observations and team were supported by the Swiss National Science Foundation (PP00P2-163967 and PP00P2-190080), the Centre for Space and Habitability (CSH) of the University of Bern, the National Centre for Competence in Research PlanetS, supported by the Swiss National Science Foundation (SNSF), and UNAM PAPIIT-IG101321. This work makes use of observations from the LCOGT network. Part of the LCOGT telescope time was granted by NOIRLab through the Mid-Scale Innovations Program (MSIP). MSIP is funded by NSF. This research has made use of the Exoplanet Follow-up Observation Program (ExoFOP; DOI: 10.26134/ExoFOP5) website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Funding for the TESS mission is provided by NASA\u2019s Science Mission Directorate. This work is partly supported by JSPS KAKENHI Grant Numbers JP17H04574, JP18H05439, JP 18H05442, JP19K14783, JP20K14521, JP21H00035, JP21K13955, JP21K20376, Grant-in-Aid for JSPS Fellows, Grant Number JP20J21872, JST CREST Grant Number JPMJCR1761, and Astrobiology Center SATELLITE Research project AB022006. This article is based on observations made with the MuSCAT2 instrument, developed by ABC, at Telescopio Carlos S\u00E1nchez operated on the island of Tenerife by the IAC in the Spanish Observatorio del Teide. M.T. is supported by JSPS KAKENHI grant Nos.18H05442. C.D. acknowledges support from the Swiss National Science Foundation under grant TMSGI2_211313. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE 1746045. G.S. acknowledges support provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51519.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. J.R.M. and B.L.C.M. acknowledge continuous grants from the brazilian funding agencies CAPES (Finance Code 001) and CNPq. The material is based upon work supported by NASA under award number 80GSFC21M0002.
We are grateful to the ESO/La Silla staff for their continuous support. We acknowledge funding from the European Research Council under the ERC Grant Agreement n. 337591-ExTrA. This paper includes data collected by the TESS mission. Funding for the TESS mission is provided by the NASA Explorer Program. We acknowledge the use of public TESS Alert data from the pipelines at the TESS Science Office and at the TESS Science Processing Operations Center. Resources supporting this work were provided by the NASA High-End Computing (HEC) program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center for the production of the SPOC data products. We thank the Swiss National Science Foundation (SNSF) and the Geneva University for their continuous support to our planet search programs. This work has been in particular carried out in the frame of the National Centre for Competence in Research \u2018PlanetS\u2019 supported by the Swiss National Science Foundation (SNSF). This work made use of tpfplotter by J. Lillo-Box (publicly available in www.github.com/jlillo/tpfplotter), which also made use of the python packages astropy, lightkurve, matplotlib and numpy. This research was carried out in part at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (NASA). Some of the observations in this paper made use of the High-Resolution Imaging instrument Zorro and were obtained under Gemini LLP Proposal Number: GN/S-2021A-LP-105. Zorro was funded by the NASA Exoplanet Exploration Program and built at the NASA Ames Research Center by Steve B. Howell, Nic Scott, Elliott P. Horch, and Emmett Quigley. Zorro was mounted on the Gemini South telescope of the international Gemini Observatory, a program of NSF\u2019s OIR Lab, which is managed by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation on behalf of the Gemini partnership: the National Science Foundation (United States), National Research Council (Canada), Agencia Nacional de Investigaci\u00F3n y Desarrollo (Chile), Ministerio de Ciencia, Tecnolog\u00EDa e Innovaci\u00F3n (Argentina), Minist\u00E9rio da Ci\u00EAncia, Tecnologia, Inova\u00E7\u00F5es e Comunica\u00E7\u00F5es (Brazil), and Korea Astronomy and Space Science Institute (Republic of Korea). Some observations in this paper were obtained with MAROON-X, a visitor instrument on the Gemini North telescope, located within the Maunakea Science Reserve and adjacent to the summit of Maunakea. We are grateful for the privilege of observing the Universe from a place that is unique in both its astronomical quality and its cultural significance. This work is based upon observations carried out at the Observatorio Astron\u00F3mico Nacional on the Sierra de San Pedro M\u00E1rtir (OAN-SPM), Baja California, M\u00E9xico. SAINT-EX observations and team were supported by the Swiss National Science Foundation (PP00P2-163967 and PP00P2-190080), the Centre for Space and Habitability (CSH) of the University of Bern, the National Centre for Competence in Research PlanetS, supported by the Swiss National Science Foundation (SNSF), and UNAM PAPIIT-IG101321. This work makes use of observations from the LCOGT network. Part of the LCOGT telescope time was granted by NOIRLab through the Mid-Scale Innovations Program (MSIP). MSIP is funded by NSF. This research has made use of the Exoplanet Follow-up Observation Program (ExoFOP; DOI: 10.26134/ExoFOP5) website, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program. Funding for the TESS mission is provided by NASA\u2019s Science Mission Directorate. This work is partly supported by JSPS KAKENHI Grant Numbers JP17H04574, JP18H05439, JP 18H05442, JP19K14783, JP20K14521, JP21H00035, JP21K13955, JP21K20376, Grant-in-Aid for JSPS Fellows, Grant Number JP20J21872, JST CREST Grant Number JPMJCR1761, and Astrobiology Center SATELLITE Research project AB022006. This article is based on observations made with the MuSCAT2 instrument, developed by ABC, at Telescopio Carlos S\u00E1nchez operated on the island of Tenerife by the IAC in the Spanish Observatorio del Teide. M.T. is supported by JSPS KAKENHI grant Nos.18H05442. C.D. acknowledges support from the Swiss National Science Foundation under grant TMSGI2_211313. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE 1746045. G.S. acknowledges support provided by NASA through the NASA Hubble Fellowship grant HST-HF2-51519.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. J.R.M. and B.L.C.M. acknowledge continuous grants from the brazilian funding agencies CAPES (Finance Code 001) and CNPq. The material is based upon work supported by NASA under award number 80GSFC21M0002.

Muestra la fuente de financiamiento declarada en la publicación.