中文
相关论文

相关论文: The CARMENES search for exoplanets around M dwarfs…

200 篇论文

Previous simulations predicted the activity-induced radial-velocity (RV) variations of M dwarfs to range from $\sim1$ cm/s to $\sim1$ km/s, depending on various stellar and activity parameters. We investigate the observed relations between…

Radial velocities (RVs) measured from high-resolution stellar spectra are routinely used to detect and characterise orbiting exoplanet companions. The different lines present in stellar spectra are created by several species, which are…

Current exoplanet surveys using the radial velocity (RV) technique are targeting M dwarfs because any habitable zone terrestrial-mass planets will induce a high RV and orbit on shorter periods than for more massive stars. One of the main…

The CARMENES instrument is searching for periodic radial-velocity (RV) variations of M dwarfs, which are induced by orbiting planets. However, there are other potential sources of such variations, including rotational modulation caused by…

For years, the standard procedure to measure radial velocities (RVs) of spectral observations consisted in cross-correlating the spectra with a binary mask, that is, a simple stellar template that contains information on the position and…

The CARMENES survey is searching for Earth-like planets orbiting M dwarfs using the radial velocity method. Studying the stellar activity of the target stars is important to avoid false planet detections and to improve our understanding of…

Context. Current exoplanet surveys are focused on detecting small exoplanets orbiting in the liquid-water habitable zones of their host stars. Despite the recent significant advancements in instrumental developments, the current limitation…

The CARMENES instrument was conceived to deliver high-accuracy radial velocity (RV) measurements with long-term stability to search for temperate rocky planets around a sample of nearby cool stars. The broad wavelength coverage was designed…

地球与行星天体物理 · 物理学 2023-03-01 I. Ribas , A. Reiners , M. Zechmeister , J. A. Caballero , J. C. Morales , S. Sabotta , D. Baroch , P. J. Amado , A. Quirrenbach , M. Abril , J. Aceituno , G. Anglada-Escudé , M. Azzaro , D. Barrado , V. J. S. Béjar , D. Benítez de Haro , G. Bergond , P. Bluhm , R. Calvo Ortega , C. Cardona Guillén , P. Chaturvedi , C. Cifuentes , J. Colomé , D. Cont , M. Cortés-Contreras , S. Czesla , E. Díez-Alonso , S. Dreizler , C. Duque-Arribas , N. Espinoza , M. Fernández , B. Fuhrmeister , D. Galadí-Enríquez , A. García-López , E. González-Álvarez , J. I. González Hernández , E. W. Guenther , E. de Guindos , A. P. Hatzes , Th. Henning , E. Herrero , D. Hintz , Á. L. Huelmo , S. V. Jeffers , E. N. Johnson , E. de Juan , A. Kaminski , J. Kemmer , J. Khaimova , S. Khalafinejad , D. Kossakowski , M. Kürster , F. Labarga , M. Lafarga , S. Lalitha , M. Lampón , J. Lillo-Box , N. Lodieu , M. J. López González , M. López-Puertas , R. Luque , H. Magán , L. Mancini , E. Marfil , E. L. Martín , S. Martín-Ruiz , K. Molaverdikhani , D. Montes , E. Nagel , L. Nortmann , G. Nowak , E. Pallé , V. M. Passegger , A. Pavlov , S. Pedraz , V. Perdelwitz , M. Perger , A. Ramón-Ballesta , S. Reffert , D. Revilla , E. Rodríguez , C. Rodríguez-López , S. Sadegi , M. Á. Sánchez Carrasco , A. Sánchez-López , J. Sanz-Forcada , S. Schäfer , M. Schlecker , J. H. M. M. Schmitt , P. Schöfer , A. Schweitzer , W. Seifert , Y. Shan , S. L. Skrzypinski , E. Solano , O. Stahl , M. Stangret , S. Stock , J. Stürmer , H. M. Tabernero , L. Tal-Or , T. Trifonov , S. Vanaverbeke , F. Yan , M. R. Zapatero Osorio

CARMENES is a spectrograph for radial velocity surveys of M dwarfs with the aim of detecting Earth-mass planets orbiting in the habitable zones of their host stars. To ensure an optimal use of the CARMENES Guaranteed Time Observations, in…

The CARMENES radial velocity (RV) survey is observing 324 M dwarfs to search for any orbiting planets. In this paper, we present the survey sample by publishing one CARMENES spectrum for each M dwarf. These spectra cover the wavelength…

太阳与恒星天体物理 · 物理学 2018-04-25 A. Reiners , M. Zechmeister , J. A. Caballero , I. Ribas , J. C. Morales , S. V. Jeffers , P. Schöfer , L. Tal-Or , A. Quirrenbach , P. J. Amado , A. Kaminski , W. Seifert , M. Abril , J. Aceituno , F. J. Alonso-Floriano , M. Ammler-von Eiff , R. Antona , G. Anglada-Escudé , H. Anwand-Heerwart , B. Arroyo-Torres , M. Azzaro , D. Baroch , D. Barrado , F. F. Bauer , S. Becerril , V. J. S. Béjar , D. Benítez , Z. M. Berdiñas , G. Bergond , M. Blümcke , M. Brinkmöller , C. del Burgo , J. Cano , M. C. Cárdenas Vázquez , E. Casal , C. Cifuentes , A. Claret , J. Colomé , M. Cortés-Contreras , S. Czesla , E. Díez-Alonso , S. Dreizler , C. Feiz , M. Fernández , I. M. Ferro , B. Fuhrmeister , D. Galadí-Enríquez , A. Garcia-Piquer , M. L. García Vargas , L. Gesa , V. Gómez , Galera , J. I. González Hernández , R. González-Peinado , U. Grözinger , S. Grohnert , J. Guàrdia , E. W. Guenther , A. Guijarro , E. de Guindos , J. Gutiérrez-Soto , H. -J. Hagen , A. P. Hatzes , P. H. Hauschildt , R. P. Hedrosa , J. Helmling , Th. Henning , I. Hermelo , R. Hernández Arabí , L. Hernández Castaño , F. Hernández Hernando , E. Herrero , A. Huber , P. Huke , E. Johnson , E. de Juan , M. Kim , R. Klein , J. Klüter , A. Klutsch , M. Kürster , M. Lafarga , A. Lamert , M. Lampón , L. M. Lara , W. Laun , U. Lemke , R. Lenzen , R. Launhardt , M. López del Fresno , J. López-González , M. López-Puertas , J. F. López Salas , J. López-Santiago , R. Luque , H. Magán Madinabeitia , U. Mall , L. Mancini , H. Mandel , E. Marfil , J. A. Marín Molina , D. Maroto , Fernández , E. L. Martín , S. Martín-Ruiz , C. J. Marvin , R. J. Mathar , E. Mirabet , D. Montes , M. E. Moreno-Raya , A. Moya , R. Mundt , E. Nagel , V. Naranjo , L. Nortmann , G. Nowak , A. Ofir , R. Oreiro , E. Pallé , J. Panduro , J. Pascual , V. M. Passegger , A. Pavlov , S. Pedraz , A. Pérez-Calpena , D. Pérez Medialdea , M. Perger , M. A. C. Perryman , M. Pluto , O. Rabaza , A. Ramón , R. Rebolo , P. Redondo , S. Reffert , S. Reinhart , P. Rhode , H. -W. Rix , F. Rodler , E. Rodríguez , C. Rodríguez-López , A. Rodríguez Trinidad , R. -R. Rohloff , A. Rosich , S. Sadegi , E. Sánchez-Blanco , M. A. Sánchez Carrasco , A. Sánchez-López , J. Sanz-Forcada , P. Sarkis , L. F. Sarmiento , S. Schäfer , J. H. M. M. Schmitt , J. Schiller , A. Schweitzer , E. Solano , O. Stahl , J. B. P. Strachan , J. Stürmer , J. C. Suárez , H. M. Tabernero , M. Tala , T. Trifonov , S. M. Tulloch , R. G. Ulbrich , G. Veredas , J. I. Vico Linares , F. Vilardell , K. Wagner , J. Winkler , V. Wolthoff , W. Xu , F. Yan , M. R. Zapatero Osorio

It is clearly established that the Sun has an 11-year cycle that is caused by its internal magnetic field. This cycle is also observed in a sample of M dwarfs. In the framework of exoplanet detection or atmospheric characterisation of…

Context. Variability caused by stellar activity represents a challenge to the discovery and characterization of terrestrial exoplanets and complicates the interpretation of atmospheric planetary signals. Aims. We aim to use a detailed…

Aims. Our goals are to characterise the kinematic properties and to identify young and old stars among the M dwarfs of the CARMENES input catalogue. Methods. We compiled the spectral types, proper motions, distances, and radial velocities…

A multitude of spectral activity indicators are routinely computed nowadays from the spectra generated as part of planet-hunting radial velocity surveys. Searching for shared periods among them can help to robustly identify astrophysical…

Due to their low mass and luminosity, M dwarfs are ideal targets if one hopes to find low-mass planets similar to Earth by using the radial velocity (RV) method. However, stellar magnetic cycles could add noise or even mimic the RV signal…

太阳与恒星天体物理 · 物理学 2015-06-04 J. Gomes da Silva , N. C. Santos , X. Bonfils , X. Delfosse , T. Forveille , S. Udry , X. Dumusque , C. Lovis

Stellar rotation is closely linked to both age and magnetic activity. Through gyrochronology, it provides a means to estimate stellar ages and trace the evolution of planetary systems, and it is also crucial to constrain and correct stellar…

Radial-velocity (RV) jitter caused by stellar magnetic activity is an important factor in state-of-the-art exoplanet discovery surveys such as CARMENES. Stellar rotation, along with heterogeneities in the photosphere and chromosphere caused…

The new CARMENES instrument comprises two high-resolution and high-stability spectrographs that are used to search for habitable planets around M dwarfs in the visible and near-infrared regime via the Doppler technique. Characterising our…

‹ 上一页 1 2 3 10 下一页 ›