The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines

We use spectra from CARMENES, the Calar Alto high-Resolution search for M dwarfs with Exo-earths with Near-infrared and optical Echelle Spectrographs, to search for periods in chromospheric indices in 16 M0-M2 dwarfs. We measure spectral indices in the Hα, the Ca II infrared triplet (IRT), and the N...

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Autores: Fuhrmeister, Birgit, Czesla, S., Schmitt, Jürgen H. M. M., Johnson, E.N., Schöfer, P., Jeffers, Sandra V., Caballero, J. A., Zechmeister, Mathias, Reiners, Ansgar, Ribas, Ignasi, Amado, Pedro J., Quirrenbach, Andreas, Bauer, Florian Franz, Béjar, Victor J. S., Cortés-Contreras, M., Díez-Alonso, E., Dreizler, Stefan, Galadí-Enriquez, D., Guenther, E. W., Kaminski, Adrian, Kürster, M., Lafarga, M., Montes, David
Formato: artículo
Estado:Versión publicada
Fecha de publicación:2019
País:España
Recursos:Consejo Superior de Investigaciones Científicas (CSIC)
Repositorio:DIGITAL.CSIC. Repositorio Institucional del CSIC
OAI Identifier:oai:digital.csic.es:10261/185676
Acesso em linha:http://hdl.handle.net/10261/185676
Access Level:acceso abierto
Palavra-chave:Stars: rotation
Stars: activity
Stars: chromospheres
Stars: late-type
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network_acronym_str ES
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repository_id_str
spelling The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT linesFuhrmeister, BirgitCzesla, S.Schmitt, Jürgen H. M. M.Johnson, E.N.Schöfer, P.Jeffers, Sandra V.Caballero, J. A.Zechmeister, MathiasReiners, AnsgarRibas, IgnasiAmado, Pedro J.Quirrenbach, AndreasBauer, Florian FranzBéjar, Victor J. S.Cortés-Contreras, M.Díez-Alonso, E.Dreizler, StefanGaladí-Enriquez, D.Guenther, E. W.Kaminski, AdrianKürster, M.Lafarga, M.Montes, DavidStars: rotationStars: activityStars: chromospheresStars: late-typeWe use spectra from CARMENES, the Calar Alto high-Resolution search for M dwarfs with Exo-earths with Near-infrared and optical Echelle Spectrographs, to search for periods in chromospheric indices in 16 M0-M2 dwarfs. We measure spectral indices in the Hα, the Ca II infrared triplet (IRT), and the Na I D lines to study which of these indices are best-suited to finding rotation periods in these stars. Moreover, we test a number of different period-search algorithms, namely the string length method, the phase dispersion minimisation, the generalized Lomb-Scargle periodogram, and the Gaussian process regression with quasi-periodic kernel. We find periods in four stars using Hα and in five stars using the Ca II IRT, two of which have not been found before. Our results show that both Hα and the Ca II IRT lines are well suited for period searches, with the Ca II IRT index performing slightly better than Hα. Unfortunately, the Na I D lines are strongly affected by telluric airglow, and we could not find any rotation period using this index. Further, different definitions of the line indices have no major impact on the results. Comparing the different search methods, the string length method and the phase dispersion minimisation perform worst, while Gaussian process models produce the smallest numbers of false positives and non-detections.© 2019 ESO.B.F. acknowledges funding by the DFG under Cz 222/1-1. CARMENES is an instrument for the Centro Astronomico Hispano-Aleman de Calar Alto (CAHA, Almeria, Spain). CARMENES is funded by the German Max-Planck-Gesellschaft (MPG), the Spanish Consejo Superior de Investigaciones Cientificas (CSIC), the European Union through FEDER/ERF FICTS-2011-02 funds, and the members of the CARMENES Consortium (Max-Planck-Institut fur Astronomie, Instituto de Astrofisica de Andalucia, Landessternwarte Konigstuhl, Institut de Ciencies de l'Espai, Institut fur Astrophysik Gottingen, Universidad Complutense de Madrid, Thuringer Landessternwarte Tautenburg, Instituto de Astrofisica de Canarias, Hamburger Sternwarte, Centro de Astrobiologia and Centro Astronomico Hispano-Aleman), with additional contributions by the Spanish Ministry of Economy, the German Science Foundation through the Major Research Instrumentation Programme and DFG Research Unit FOR2544 >Blue Planets around Red Stars>, the Klaus Tschira Stiftung, the states of Baden-Wurttemberg and Niedersachsen, and by the Junta de Andalucia.Peer ReviewedEDP SciencesMax Planck SocietyGerman Research FoundationJunta de AndalucíaMinisterio de Ciencia e Innovación (España)European CommissionConsejo Superior de Investigaciones Científicas (España)Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]2019201920192019info:eu-repo/semantics/articlehttp://purl.org/coar/resource_type/c_6501Publisher's versioninfo:eu-repo/semantics/publishedVersionhttp://hdl.handle.net/10261/185676reponame:DIGITAL.CSIC. Repositorio Institucional del CSICinstname:Consejo Superior de Investigaciones Científicas (CSIC)InglésSíinfo:eu-repo/semantics/openAccessoai:digital.csic.es:10261/1856762026-05-22T06:33:51Z
dc.title.none.fl_str_mv The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
title The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
spellingShingle The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
Fuhrmeister, Birgit
Stars: rotation
Stars: activity
Stars: chromospheres
Stars: late-type
title_short The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
title_full The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
title_fullStr The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
title_full_unstemmed The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
title_sort The CARMENES search for exoplanets around M dwarfs: Period search in H α, Na i D, and Ca II IRT lines
dc.creator.none.fl_str_mv Fuhrmeister, Birgit
Czesla, S.
Schmitt, Jürgen H. M. M.
Johnson, E.N.
Schöfer, P.
Jeffers, Sandra V.
Caballero, J. A.
Zechmeister, Mathias
Reiners, Ansgar
Ribas, Ignasi
Amado, Pedro J.
Quirrenbach, Andreas
Bauer, Florian Franz
Béjar, Victor J. S.
Cortés-Contreras, M.
Díez-Alonso, E.
Dreizler, Stefan
Galadí-Enriquez, D.
Guenther, E. W.
Kaminski, Adrian
Kürster, M.
Lafarga, M.
Montes, David
author Fuhrmeister, Birgit
author_facet Fuhrmeister, Birgit
Czesla, S.
Schmitt, Jürgen H. M. M.
Johnson, E.N.
Schöfer, P.
Jeffers, Sandra V.
Caballero, J. A.
Zechmeister, Mathias
Reiners, Ansgar
Ribas, Ignasi
Amado, Pedro J.
Quirrenbach, Andreas
Bauer, Florian Franz
Béjar, Victor J. S.
Cortés-Contreras, M.
Díez-Alonso, E.
Dreizler, Stefan
Galadí-Enriquez, D.
Guenther, E. W.
Kaminski, Adrian
Kürster, M.
Lafarga, M.
Montes, David
author_role author
author2 Czesla, S.
Schmitt, Jürgen H. M. M.
Johnson, E.N.
Schöfer, P.
Jeffers, Sandra V.
Caballero, J. A.
Zechmeister, Mathias
Reiners, Ansgar
Ribas, Ignasi
Amado, Pedro J.
Quirrenbach, Andreas
Bauer, Florian Franz
Béjar, Victor J. S.
Cortés-Contreras, M.
Díez-Alonso, E.
Dreizler, Stefan
Galadí-Enriquez, D.
Guenther, E. W.
Kaminski, Adrian
Kürster, M.
Lafarga, M.
Montes, David
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.contributor.none.fl_str_mv Max Planck Society
German Research Foundation
Junta de Andalucía
Ministerio de Ciencia e Innovación (España)
European Commission
Consejo Superior de Investigaciones Científicas (España)
Consejo Superior de Investigaciones Científicas [https://ror.org/02gfc7t72]
dc.subject.none.fl_str_mv Stars: rotation
Stars: activity
Stars: chromospheres
Stars: late-type
topic Stars: rotation
Stars: activity
Stars: chromospheres
Stars: late-type
description We use spectra from CARMENES, the Calar Alto high-Resolution search for M dwarfs with Exo-earths with Near-infrared and optical Echelle Spectrographs, to search for periods in chromospheric indices in 16 M0-M2 dwarfs. We measure spectral indices in the Hα, the Ca II infrared triplet (IRT), and the Na I D lines to study which of these indices are best-suited to finding rotation periods in these stars. Moreover, we test a number of different period-search algorithms, namely the string length method, the phase dispersion minimisation, the generalized Lomb-Scargle periodogram, and the Gaussian process regression with quasi-periodic kernel. We find periods in four stars using Hα and in five stars using the Ca II IRT, two of which have not been found before. Our results show that both Hα and the Ca II IRT lines are well suited for period searches, with the Ca II IRT index performing slightly better than Hα. Unfortunately, the Na I D lines are strongly affected by telluric airglow, and we could not find any rotation period using this index. Further, different definitions of the line indices have no major impact on the results. Comparing the different search methods, the string length method and the phase dispersion minimisation perform worst, while Gaussian process models produce the smallest numbers of false positives and non-detections.© 2019 ESO.
publishDate 2019
dc.date.none.fl_str_mv 2019
2019
2019
2019
dc.type.none.fl_str_mv info:eu-repo/semantics/article
http://purl.org/coar/resource_type/c_6501
Publisher's version
info:eu-repo/semantics/publishedVersion
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/10261/185676
url http://hdl.handle.net/10261/185676
dc.language.none.fl_str_mv Inglés
language_invalid_str_mv Inglés
dc.relation.none.fl_str_mv
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.publisher.none.fl_str_mv EDP Sciences
publisher.none.fl_str_mv EDP Sciences
dc.source.none.fl_str_mv reponame:DIGITAL.CSIC. Repositorio Institucional del CSIC
instname:Consejo Superior de Investigaciones Científicas (CSIC)
instname_str Consejo Superior de Investigaciones Científicas (CSIC)
reponame_str DIGITAL.CSIC. Repositorio Institucional del CSIC
collection DIGITAL.CSIC. Repositorio Institucional del CSIC
repository.name.fl_str_mv
repository.mail.fl_str_mv
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