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Verfasst von:Toledo-Padrón, Borja [VerfasserIn]   i
 Mascareño, A. Suárez [VerfasserIn]   i
 Hernández, J. I. González [VerfasserIn]   i
 Rebolo, R. [VerfasserIn]   i
 Pinamonti, M. [VerfasserIn]   i
 Perger, M. [VerfasserIn]   i
 Scandariato, G. [VerfasserIn]   i
 Damasso, M. [VerfasserIn]   i
 Sozzetti, A. [VerfasserIn]   i
 Maldonado, J. [VerfasserIn]   i
 Desidera, S. [VerfasserIn]   i
 Ribas, I. [VerfasserIn]   i
 Micela, G. [VerfasserIn]   i
 Affer, L. [VerfasserIn]   i
 González-Alvarez, E. [VerfasserIn]   i
 Leto, G. [VerfasserIn]   i
 Pagano, I. [VerfasserIn]   i
 Sánchez, R. Zanmar [VerfasserIn]   i
 Giacobbe, P. [VerfasserIn]   i
 Herrero, E. [VerfasserIn]   i
 Morales, J. C. [VerfasserIn]   i
 Amado, P. J. [VerfasserIn]   i
 Caballero, J. A. [VerfasserIn]   i
 Quirrenbach, Andreas [VerfasserIn]   i
 Reiners, A. [VerfasserIn]   i
 Zechmeister, M. [VerfasserIn]   i
Titel:A super-earth on a close-in orbit around the M1V star GJ 740
Titelzusatz:a HADES and CARMENES collaboration
Verf.angabe:B. Toledo-Padrón, A. Suárez Mascareño, J.I. González Hernández, R. Rebolo, M. Pinamonti, M. Perger, G. Scandariato, M. Damasso, A. Sozzetti, J. Maldonado, S. Desidera, I. Ribas, G. Micela, L. Affer, E. González-Alvarez, G. Leto, I. Pagano, R. Zanmar Sánchez, P. Giacobbe, E. Herrero, J.C. Morales, P.J. Amado, J.A. Caballero, A. Quirrenbach, A. Reiners, and M. Zechmeister
E-Jahr:2021
Jahr:10 February 2021
Umfang:15 S.
Teil:volume:648
 year:2021
 elocationid:A20
 pages:1-15
 extent:15
Fussnoten:Gesehen am 02.08.2021
Titel Quelle:Enthalten in: Astronomy and astrophysics
Ort Quelle:Les Ulis : EDP Sciences, 1969
Jahr Quelle:2021
Band/Heft Quelle:648(2021), Artikel-ID A20, Seite 1-15
ISSN Quelle:1432-0746
Abstract:<i>Context.<i/> M-dwarfs have proven to be ideal targets for planetary radial velocity (RV) searches due to their higher planet-star mass contrast, which favors the detection of low-mass planets. The abundance of super-Earth and Earth-like planets detected around this type of star motivates further such research on hosts without reported planetary companions.<i>Aims.<i/> The HADES and CARMENES programs are aimed at carrying out extensive searches of exoplanetary systems around M-type stars in the northern hemisphere, allowing us to address, in a statistical sense, the properties of the planets orbiting these objects. In this work, we perform a spectroscopic and photometric study of one of the program stars (GJ 740), which exhibits a short-period RV signal that is compatible with a planetary companion.<i>Methods.<i/> We carried out a spectroscopic analysis based on 129 HARPS-N spectra taken over a time span of 6 yr combined with 57 HARPS spectra taken over 4 yr, as well as 32 CARMENES spectra taken during more than 1 yr, resulting in a dataset with a time coverage of 10 yr. We also relied on 459 measurements from the public ASAS survey with a time-coverage of 8 yr, along with 5 yr of photometric magnitudes from the EXORAP project taken in the <i>V<i/>, <i>B<i/>, <i>R<i/>, and <i>I<i/> filters to carry out a photometric study. Both analyses were made using Markov chain Monte Carlo simulations and Gaussian process regression to model the activity of the star.<i>Results.<i/> We present the discovery of a short-period super-Earth with an orbital period of 2.37756 d and a minimum mass of 2.96 <i>M<i/><sub>⊕<sub/>. We offer an update to the previously reported characterization of the magnetic cycle and rotation period of the star, obtaining values of <i>P<i/><sub>rot<sub/> = 35.563 ± 0.071 d and <i>P<i/><sub>cycle<sub/> = 2800 ± 150 d. Furthermore, the RV time series exhibits a possibly periodic long-term signal, which might be related to a Saturn-mass planet of ~100 <i>M<i/><sub>⊕<sub/>.
DOI:doi:10.1051/0004-6361/202040099
URL:Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt.

Volltext ; Verlag: https://doi.org/10.1051/0004-6361/202040099
 Volltext: https://www.aanda.org/articles/aa/abs/2021/04/aa40099-20/aa40099-20.html
 DOI: https://doi.org/10.1051/0004-6361/202040099
Datenträger:Online-Ressource
Sprache:eng
K10plus-PPN:1765252873
Verknüpfungen:→ Zeitschrift

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