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

Autor: J. Blanco-Pozo, M. Perger, M. Damasso, G. Anglada Escudé, I. Ribas, D. Baroch, J. A. Caballero, C. Cifuentes, S. V. Jeffers, M. Lafarga, A. Kaminski, S. Kaur, E. Nagel, V. Perdelwitz, M. Pérez-Torres, A. Sozzetti, D. Viganò, P. J. Amado, G. Andreuzzi, V. J. S. Béjar, E. L. Brown, F. Del Sordo, S. Dreizler, D. Galadí-Enríquez, A. P. Hatzes, M. Kürster, A. F. Lanza, A. Melis, E. Molinari, D. Montes, M. Murgia, E. Pallé, L. Peña-Moñino, D. Perrodin, M. Pilia, E. Poretti, A. Quirrenbach, A. Reiners, A. Schweitzer, M. R. Zapatero Osorio, M. Zechmeister

This is an Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provid

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::cf77027919a5f79d8528d286d3a46de1

Detailed stellar activity analysis and modelling of GJ 832. Reassessment of the putative habitable zone planet GJ 832c

Autor: P. Gorrini, N. Astudillo-Defru, S. Dreizler, M. Damasso, R. F. Díaz, X. Bonfils, S. V. Jeffers, J. R. Barnes, F. Del Sordo, J.-M. Almenara, E. Artigau, F. Bouchy, D. Charbonneau, X. Delfosse, R. Doyon, P. Figueira, T. Forveille, C. A. Haswell, M. J. López-González, C. Melo, R. E. Mennickent, G. Gaisné, N. Morales Morales, F. Murgas, F. Pepe, E. Rodríguez, N. C. Santos, L. Tal-Or, Y. Tsapras, S. Udry

Publikováno v: Astronomy and Astrophysics
Digital.CSIC. Repositorio Institucional del CSIC
instname

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the orig

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::32348e210af902560bf7c57e12befb5b
https://hdl.handle.net/21.11116/0000-000C-B1E3-B

Searching for the near-infrared counterpart of Proxima c using multi-epoch high-contrast SPHERE data at VLT

Autor: Thomas Henning, Mickael Bonnefoy, Arthur Vigan, Janis Hagelberg, Gael Chauvin, Philippe Delorme, Thierry Fusco, Markus Feldt, A. Potier, A-M. Lagrange, Mario Damasso, Julien Milli, E. Sissa, Valentina D'Orazi, R. Galicher, Alessandro Sozzetti, C. Lazzoni, T. O. B. Schmidt, L. Rodet, E. Lagadec, Samantha Brown, Michael R. Meyer, Jacopo Antichi, E. L. Rickman, H. Le Coroller, Laurent M. Mugnier, F. Del Sordo, Dino Mesa, Pierre Kervella, Alice Zurlo, Faustine Cantalloube, Anthony Boccaletti, Zahed Wahhaj, Francois Wildi, Roxanne Ligi, Maud Langlois, Raffaele Gratton, Wolfgang Brandner, Marcos Suarez, Markus Janson, C. Romero, François Ménard, Judit Szulágyi, Eric Stadler, Silvano Desidera, Anne-Lise Maire

Publikováno v: Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, 2020, 638, pp.A120. ⟨10.1051/0004-6361/202037594⟩
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 638, pp.A120. ⟨10.1051/0004-6361/202037594⟩

Proxima Centauri is known to host an earth-like planet in its habitable zone; very recently a second candidate planet was proposed based on radial velocities. At quadrature, the expected projected separation of this new candidate is larger than 1 arc

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06746939673cb1420ed74958243e7f28
http://hdl.handle.net/11577/3355695