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The case of Ross 176 is a late K-type star that hosts a promising water-world candidate planet. The star has a radius of $R_*$=0.569$\pm$0.020$R_{\odot}$ and a mass of $M_{\star}$ = 0.577 $\pm$ 0.024 $M_{\odot}$. We constrained the…

We present the first planet mass measurement obtained with CRIRES+ radial velocity (RV) observations using the K-band gas cell. Our target, LHS 3844 b (TOI-136), is a transiting super-Earth with radius $R_b=1.286^{+0.043}_{-0.044}R_\oplus$…

We present the discovery of TOI-2136b, a sub-Neptune planet transiting every 7.85 days a nearby M4.5V-type star, identified through photometric measurements from the TESS mission. The host star is located $33$ pc away with a radius of…

We report the discovery of HN Lib b, a sub-Neptunian mass planet orbiting the nearby ($d \approx$ = 6.25 pc) M4.0 V star HN Lib detected by our CARMENES radial-velocity (RV) survey. We determined a planetary minimum mass of $M_\text{b}\sin…

K2-18 is a nearby M2.5 dwarf, located at 34 pc and hosting a transiting planet which was first discovered by the {\it K2} mission and later confirmed with {\it Spitzer Space Telescope} observations. With a radius of $\sim 2 \, R_{\oplus}$…

We report the detection of a transiting Earth-size planet around GJ 357, a nearby M2.5V star, using data from the Transiting Exoplanet Survey Satellite (TESS). GJ 357 b (TOI-562.01) is a transiting, hot, Earth-sized planet (Teq=525+-11 K)…

We present the bright (V$_{mag} = 9.12$), multi-planet system TOI-431, characterised with photometry and radial velocities. We estimate the stellar rotation period to be $30.5 \pm 0.7$ days using archival photometry and radial velocities.…

Earth and Planetary Astrophysics · Physics 2021-08-18 Ares Osborn , David J. Armstrong , Bryson Cale , Rafael Brahm , Robert A. Wittenmyer , Fei Dai , Ian J. M. Crossfield , Edward M. Bryant , Vardan Adibekyan , Ryan Cloutier , Karen A. Collins , E. Delgado Mena , Malcolm Fridlund , Coel Hellier , Steve B. Howell , George W. King , Jorge Lillo-Box , Jon Otegi , S. Sousa , Keivan G. Stassun , Elisabeth C. Matthews , Carl Ziegler , George Ricker , Roland Vanderspek , David W. Latham , S. Seager , Joshua N. Winn , Jon M. Jenkins , Jack S. Acton , Brett C. Addison , David R. Anderson , Sarah Ballard , David Barrado , Susana C. C. Barros , Natalie Batalha , Daniel Bayliss , Thomas Barclay , Björn Benneke , John Berberian , Francois Bouchy , Brendan P. Bowler , César Briceño , Christopher J. Burke , Matthew R. Burleigh , Sarah L. Casewell , David Ciardi , Kevin I. Collins , Benjamin F. Cooke , Olivier D. S. Demangeon , Rodrigo F. Díaz , C. Dorn , Diana Dragomir , Courtney Dressing , Xavier Dumusque , Néstor Espinoza , P. Figueira , Benjamin Fulton , E. Furlan , E. Gaidos , C. Geneser , Samuel Gill , Michael R. Goad , Erica J. Gonzales , Varoujan Gorjian , Maximilian N. Günther , Ravit Helled , Beth A. Henderson , Thomas Henning , Aleisha Hogan , Saeed Hojjatpanah , Jonathan Horner , Andrew W. Howard , Sergio Hoyer , Dan Huber , Howard Isaacson , James S. Jenkins , Eric L. N. Jensen , Andrés Jordán , Stephen R. Kane , Richard C. Kidwell , John Kielkopf , Nicholas Law , Monika Lendl , M. Lund , Rachel A. Matson , Andrew W. Mann , James McCormac , Matthew W. Mengel , Farisa Y. Morales , Louise D. Nielsen , Jack Okumura , Hugh P. Osborn , Erik A. Petigura , Peter Plavchan , Don Pollacco , Elisa V. Quintana , Liam Raynard , Paul Robertson , Mark E. Rose , Arpita Roy , Michael Reefe , Alexandre Santerne , Nuno C. Santos , Paula Sarkis , J. Schlieder , Richard P. Schwarz , Nicholas J. Scott , Avi Shporer , A. M. S. Smith , C. Stibbard , Chris Stockdale , Paul A. Strøm , Joseph D. Twicken , Thiam-Guan Tan , A. Tanner , J. Teske , Rosanna H. Tilbrook , C. G. Tinney , Stephane Udry , Jesus Noel Villaseñor , Jose I. Vines , Sharon X. Wang , Lauren M. Weiss , Richard G. West , Peter J. Wheatley , Duncan J. Wright , Hui Zhang , F. Zohrabi

Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero or up to a few percent depending on their size and orbital period. Models of thermally-driven atmospheric mass loss and of terrestrial…

Earth and Planetary Astrophysics · Physics 2020-06-17 Ryan Cloutier , Joseph E. Rodriguez , Jonathan Irwin , David Charbonneau , Keivan G. Stassun , Annelies Mortier , David W. Latham , Howard Isaacson , Andrew W. Howard , Stéphane Udry , Thomas G. Wilson , Christopher A. Watson , Matteo Pinamonti , Florian Lienhard , Paolo Giacobbe , Pere Guerra , Karen A. Collins , Allyson Beiryla , Gilbert A. Esquerdo , Elisabeth Matthews , Rachel A. Matson , Steve B. Howell , Elise Furlan , Ian J. M. Crossfield , Jennifer G. Winters , Chantanelle Nava , Kristo Ment , Eric D. Lopez , George Ricker , Roland Vanderspek , Sara Seager , Jon M. Jenkins , Eric B. Ting , Peter Tenenbaum , Alessandro Sozzetti , Lizhou Sha , Damien Ségransan , Joshua E. Schlieder , Dimitar Sasselov , Arpita Roy , Paul Robertson , Ken Rice , Ennio Poretti , Giampaolo Piotto , David Phillips , Joshua Pepper , Francesco Pepe , Emilio Molinari , Teo Mocnik , Giuseppina Micela , Michel Mayor , Aldo F. Martinez Fiorenzano , Franco Mallia , Jack Lubin , Christophe Lovis , Mercedes López-Morales , Molly R. Kosiarek , John F. Kielkopf , Stephen R. Kane , Eric L. N. Jensen , Giovanni Isopi , Daniel Huber , Michelle L. Hill , Avet Harutyunyan , Erica Gonzales , Steven Giacalone , Adriano Ghedina , Andrea Ercolino , Xavier Dumusque , Courtney D. Dressing , Mario Damasso , Paul A. Dalba , Rosario Cosentino , Dennis M. Conti , Knicole D. Colón , Kevin I. Collins , Andrew Collier Cameron , David Ciardi , Jessie Christiansen , Ashley Chontos , Massimo Cecconi , Douglas A. Caldwell , Christopher Burke , Lars Buchhave , Charles Beichman , Aida Behmard , Corey Beard , Joseph M. Akana Murphy

The Transiting Exoplanet Survey Satellite (TESS) mission identified a potential 0.88 REarth planet with a period of 7.577 days, orbiting the nearby M1V star GJ 341 (TOI 741.01). This system has already been observed by the James Webb Space…

We report the discovery and characterization of TOI-1759~b, a temperate (400 K) sub-Neptune-sized exoplanet orbiting the M~dwarf TOI-1759 (TIC 408636441). TOI-1759 b was observed by TESS to transit on sectors 16, 17 and 24, with only one…

Short- to mid-term magnetic phenomena on the stellar surface of M-type stars cannot only resemble the effects of planets in radial velocity data, but also may hide them. We analyze 145 spectroscopic HARPS-N observations of GJ 3942 taken…

M-dwarfs have proven to be ideal targets for planetary radial velocity (RV) searches due to their higher planet-star mass contrast. The HADES and CARMENES programs aim to carry out extensive searches of exoplanetary systems around this type…

Recent discoveries of Earth-sized planets transiting nearby M dwarfs have made it possible to characterize the atmospheres of terrestrial planets via follow-up spectroscopic observations. However, the number of such planets receiving low…

Earth and Planetary Astrophysics · Physics 2024-05-24 M. Kuzuhara , A. Fukui , J. H. Livingston , J. A. Caballero , J. P. de Leon , T. Hirano , Y. Kasagi , F. Murgas , N. Narita , M. Omiya , Jaume Orell-Miquel , E. Palle , Q. Changeat , E. Esparza-Borges , H. Harakawa , C. Hellier , Yasunori Hori , Kai Ikuta , H. T. Ishikawa , T. Kodama , T. Kotani , T. Kudo , J. C. Morales , M. Mori , E. Nagel , H. Parviainen , V. Perdelwitz , A. Reiners , I. Ribas , J. Sanz-Forcada , B. Sato , A. Schweitzer , H. M. Tabernero , T. Takarada , T. Uyama , N. Watanabe , M. Zechmeister , N. Abreu García , W. Aoki , C. Beichman , V. J. S. Béjar , T. D. Brandt , Y. Calatayud-Borras , I. Carleo , D. Charbonneau , K. A. Collins , T. Currie , J. P. Doty , S. Dreizler , G. Fernández-Rodríguez , I. Fukuda , D. Galán , S. Geraldía-González , J. González-Garcia , Y. Hayashi , C. Hedges , T. Henning , K. Hodapp , M. Ikoma , K. Isogai , S. Jacobson , M. Janson , J. M. Jenkins , T. Kagetani , E. Kambe , Y. Kawai , K. Kawauchi , E. Kokubo , M. Konishi , J. Korth , V. Krishnamurthy , T. Kurokawa , N. Kusakabe , J. Kwon , A. Laza-Ramos , F. Libotte , R. Luque , A. Madrigal-Aguado , Y. Matsumoto , D. Mawet , M. W. McElwain , P. P. Meni Gallardo , G. Morello , S. Mu~noz Torres , J. Nishikawa , S. K. Nugroho , M. Ogihara , A. Pel'aez-Torres , D. Rapetti , M. S'anchez-Benavente , M. Schlecker , S. Seager , E. Serabyn , T. Serizawa , M. Stangret , A. Takahashi , H. Teng , M. Tamura , Y. Terada , A. Ueda , T. Usuda , R. Vanderspek , S. Vievard , D. Watanabe , J. N. Winn , M. R. Zapatero Osorio

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…

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