The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data

[Context] Detecting a planetary companion in a short-period orbit through radio emission from the interaction with its host star is a new prospect in exoplanet science. Recently, a tantalising signal was found close to the low-mass stellar system GJ 1151 using LOFAR observations.

Detalhes bibliográficos
Autores: Blanco-Pozo, J., Perger, M., Damasso, M., Anglada-Escudé, Guillem, Ribas, Ignasi, Baroch, David, Caballero, J. A., Cifuentes, C., Jeffers, Sandra V., Lafarga, M., Kaminski, Adrian, Kaur, Simranpreet, Nagel, Evangelos, Perdelwitz, Volker, Pérez-Torres, Miguel A., Sozzetti, Alessandro, Viganò, Daniele, Amado, Pedro J., Andreuzzi, G., Béjar, Victor J. S., Brown, E. L., Del Sordo, Fabio, Dreizler, Stefan, Galadí-Enriquez, D., Hatzes, Artie P., Kürster, M., Lanza, A. F., Melis, A., Molinari, Emilio, Montes, David, Murgia, M., Pallé, Enric, Peña-Moñino, Luis, Perrodin, D., Pilia, Maura, Poretti, Ennio, Quirrenbach, Andreas, Reiners, Ansgar, Schweitzer, Andreas, Zapatero Osorio, María Rosa, Zechmeister, Mathias
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2023
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/310466
Acesso em linha:http://hdl.handle.net/10261/310466
Access Level:acceso abierto
Palavra-chave:Stars: late-type
Stars: individual: GJ 1151
Techniques: radial velocities
Planets and satellites: detection
Stars: activity
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dc.title.none.fl_str_mv The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
title The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
spellingShingle The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
Blanco-Pozo, J.
Stars: late-type
Stars: individual: GJ 1151
Techniques: radial velocities
Planets and satellites: detection
Stars: activity
title_short The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
title_full The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
title_fullStr The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
title_full_unstemmed The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
title_sort The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data
dc.creator.none.fl_str_mv Blanco-Pozo, J.
Perger, M.
Damasso, M.
Anglada-Escudé, Guillem
Ribas, Ignasi
Baroch, David
Caballero, J. A.
Cifuentes, C.
Jeffers, Sandra V.
Lafarga, M.
Kaminski, Adrian
Kaur, Simranpreet
Nagel, Evangelos
Perdelwitz, Volker
Pérez-Torres, Miguel A.
Sozzetti, Alessandro
Viganò, Daniele
Amado, Pedro J.
Andreuzzi, G.
Béjar, Victor J. S.
Brown, E. L.
Del Sordo, Fabio
Dreizler, Stefan
Galadí-Enriquez, D.
Hatzes, Artie P.
Kürster, M.
Lanza, A. F.
Melis, A.
Molinari, Emilio
Montes, David
Murgia, M.
Pallé, Enric
Peña-Moñino, Luis
Perrodin, D.
Pilia, Maura
Poretti, Ennio
Quirrenbach, Andreas
Reiners, Ansgar
Schweitzer, Andreas
Zapatero Osorio, María Rosa
Zechmeister, Mathias
author Blanco-Pozo, J.
author_facet Blanco-Pozo, J.
Perger, M.
Damasso, M.
Anglada-Escudé, Guillem
Ribas, Ignasi
Baroch, David
Caballero, J. A.
Cifuentes, C.
Jeffers, Sandra V.
Lafarga, M.
Kaminski, Adrian
Kaur, Simranpreet
Nagel, Evangelos
Perdelwitz, Volker
Pérez-Torres, Miguel A.
Sozzetti, Alessandro
Viganò, Daniele
Amado, Pedro J.
Andreuzzi, G.
Béjar, Victor J. S.
Brown, E. L.
Del Sordo, Fabio
Dreizler, Stefan
Galadí-Enriquez, D.
Hatzes, Artie P.
Kürster, M.
Lanza, A. F.
Melis, A.
Molinari, Emilio
Montes, David
Murgia, M.
Pallé, Enric
Peña-Moñino, Luis
Perrodin, D.
Pilia, Maura
Poretti, Ennio
Quirrenbach, Andreas
Reiners, Ansgar
Schweitzer, Andreas
Zapatero Osorio, María Rosa
Zechmeister, Mathias
author_role author
author2 Perger, M.
Damasso, M.
Anglada-Escudé, Guillem
Ribas, Ignasi
Baroch, David
Caballero, J. A.
Cifuentes, C.
Jeffers, Sandra V.
Lafarga, M.
Kaminski, Adrian
Kaur, Simranpreet
Nagel, Evangelos
Perdelwitz, Volker
Pérez-Torres, Miguel A.
Sozzetti, Alessandro
Viganò, Daniele
Amado, Pedro J.
Andreuzzi, G.
Béjar, Victor J. S.
Brown, E. L.
Del Sordo, Fabio
Dreizler, Stefan
Galadí-Enriquez, D.
Hatzes, Artie P.
Kürster, M.
Lanza, A. F.
Melis, A.
Molinari, Emilio
Montes, David
Murgia, M.
Pallé, Enric
Peña-Moñino, Luis
Perrodin, D.
Pilia, Maura
Poretti, Ennio
Quirrenbach, Andreas
Reiners, Ansgar
Schweitzer, Andreas
Zapatero Osorio, María Rosa
Zechmeister, Mathias
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
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author
author
author
author
author
author
author
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author
author
author
author
author
author
author
author
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author
author
dc.contributor.none.fl_str_mv Ministerio de Ciencia e Innovación (España)
European Commission
European Research Council
Ministerio de Ciencia, Innovación y Universidades (España)
Agencia Estatal de Investigación (España)
Junta de Andalucía
Max Planck Society
Consejo Superior de Investigaciones Científicas (España)
European Space Agency
Generalitat de Catalunya
Ministerio de Economía y Competitividad (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Stars: late-type
Stars: individual: GJ 1151
Techniques: radial velocities
Planets and satellites: detection
Stars: activity
topic Stars: late-type
Stars: individual: GJ 1151
Techniques: radial velocities
Planets and satellites: detection
Stars: activity
description [Context] Detecting a planetary companion in a short-period orbit through radio emission from the interaction with its host star is a new prospect in exoplanet science. Recently, a tantalising signal was found close to the low-mass stellar system GJ 1151 using LOFAR observations.
publishDate 2023
dc.date.none.fl_str_mv 2023
2023
2023
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This work has made use of data from the European Space Agency (ESA) mission Gaia: https://www.cosmos.esa.int/gaia
The data were processed by the Gaia Data Processing and Analysis Consortium (DPAC) https://www.cosmos.esa.int/web/gaia/ dpac/consortium
http://dx.doi.org/10.1051/0004-6361/202245053

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publisher.none.fl_str_mv EDP Sciences
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spelling The CARMENES search for exoplanets around M dwarfs: A long-period planet around GJ 1151 measured with CARMENES and HARPS-N dataBlanco-Pozo, J.Perger, M.Damasso, M.Anglada-Escudé, GuillemRibas, IgnasiBaroch, DavidCaballero, J. A.Cifuentes, C.Jeffers, Sandra V.Lafarga, M.Kaminski, AdrianKaur, SimranpreetNagel, EvangelosPerdelwitz, VolkerPérez-Torres, Miguel A.Sozzetti, AlessandroViganò, DanieleAmado, Pedro J.Andreuzzi, G.Béjar, Victor J. S.Brown, E. L.Del Sordo, FabioDreizler, StefanGaladí-Enriquez, D.Hatzes, Artie P.Kürster, M.Lanza, A. F.Melis, A.Molinari, EmilioMontes, DavidMurgia, M.Pallé, EnricPeña-Moñino, LuisPerrodin, D.Pilia, MauraPoretti, EnnioQuirrenbach, AndreasReiners, AnsgarSchweitzer, AndreasZapatero Osorio, María RosaZechmeister, MathiasStars: late-typeStars: individual: GJ 1151Techniques: radial velocitiesPlanets and satellites: detectionStars: activity[Context] Detecting a planetary companion in a short-period orbit through radio emission from the interaction with its host star is a new prospect in exoplanet science. Recently, a tantalising signal was found close to the low-mass stellar system GJ 1151 using LOFAR observations.[Aims] We studied spectroscopic time-series data of GJ 1151 in order to search for planetary companions, investigate possible signatures of stellar magnetic activity, and to find possible explanations for the radio signal.[Methods] We used the combined radial velocities measured from spectra acquired with the CARMENES, HARPS-N, and HPF instruments, extracted activity indices from those spectra in order to mitigate the impact of stellar magnetic activity on the data, and performed a detailed analysis of Gaia astrometry and all available photometric time series coming from the MEarth and ASAS-SN surveys.[Results] We found a M > 10.6 M⊕ companion to GJ 1151 in a 390d orbit at a separation of 0.57 au. Evidence for a second modulation is also present; this could be due to long-term magnetic variability or a second (substellar) companion. The star shows episodes of elevated magnetic activity, one of which could be linked to the observed LOFAR radio emission. We show that it is highly unlikely that the detected GJ 1151 c, or any additional outer companion is the source of the detected signal. We cannot firmly rule out the suggested explanation of an undetected short-period planet that could be related to the radio emission, as we establish an upper limit of 1.2 M⊕ for the minimum mass. © The Authors 2023.CARMENES is an instrument at the Centro Astronómico Hispano en Andalucía (CAHA) at Calar Alto (Almería, Spain), operated jointly by the Junta de Andalucía and the Instituto de Astrofísica de Andalucía (CSIC). CARMENES was funded by the Max-Planck-Gesellschaft (MPG), the Consejo Superior de Investigaciones Científicas (CSIC), the Ministerio de Economía y Competitividad (MINECO) and the European Regional Development Fund (ERDF) through projects FICTS-2011-02, ICTS-2017-07-CAHA-4, and CAHA16-CE-3978, and the members of the CARMENES Consortium (Max-Planck-Institut für Astronomie, Instituto de Astrofísica de Andalucía, Landessternwarte Königstuhl, Institut de Ciències de l’Espai, Institut für Astrophysik Göttingen, Universidad Complutense de Madrid, Thüringer Landessternwarte Tautenburg, Instituto de Astrofísica de Canarias, Hamburger Sternwarte, Centro de Astrobiología and Centro Astronómico Hispano-Alemán), with additional contributions by the MINECO, the Deutsche Forschungsgemeinschaft through the Major Research Instrumentation Programme and Research Unit FOR2544 “Blue Planets around Red Stars”, the Klaus Tschira Stiftung, the states of Baden-Württemberg and Niedersachsen, and by the Junta de Andalucía. This work was partly based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated by the Fundación Galileo Galilei (FGG) of the Istituto Nazionale di Astrofisica (INAF) at the Observatorio del Roque de los Muchachos (La Palma, Canary Islands, Spain). We acknowledge financial support from the Agencia Estatal de Investigación of the Ministerio de Ciencia e Innovación MCIN/AEI/10.13039/501100011033 and the ERDF “A way of making Europe” through projects PID2020-120375GB-I00, PID2020-117404GB-C21, PID2019-109522GB-C5[1:4], PGC2018-098153-B-C33, AYA2016-79425-C3-1, and the Centre of Excellence “Severo Ochoa” and “María de Maeztu” awards to the Institut de Ciències de l’Espai (CEX2020-001058-M) Instituto de Astrofísica de Canarias (CEX2019-000920-S), Instituto de Astrofísica de Andalucía (SEV-2017-0709), and Centro de Astrobiología (MDM-2017-0737); the Generalitat de Catalunya/CERCA programme; the European Union through a Marie Curie Action (101030103); the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (ERC Starting Grant IMAGINE, No. 948582); the DFG through priority program SPP 1992 “Exploring the Diversity of Extrasolar Planets” (JE 701/5-1); and the Italian Space Agency (ASI) in collaboration with the Istituto Nazionale di Astrofisica under contract 2018-24-HH.0. We made use of data from the European Space Agency (ESA) mission Gaia (https://www.cosmos.esa.int/gaia), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.With funding from the Spanish government through the "Unit of Excellence Maria de Maeztu" accreditation (CEX2020-001058-M).With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (CEX2019-000920-S).With funding from the Spanish government through the "Severo Ochoa Centre of Excellence" accreditation (SEV-2017-0709)With funding from the Spanish government through the "Unit of Excellence Maria de Maeztu" accreditation (MDM-2017-0737).Peer reviewedEDP SciencesMinisterio de Ciencia e Innovación (España)European CommissionEuropean Research CouncilMinisterio de Ciencia, Innovación y Universidades (España)Agencia Estatal de Investigación (España)Junta de AndalucíaMax Planck SocietyConsejo Superior de Investigaciones Científicas (España)European Space AgencyGeneralitat de CatalunyaMinisterio de Economía y Competitividad (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]202320232023info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionapplication/pdfhttp://hdl.handle.net/10261/310466reponame:DIGITAL.CSIC. 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