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Transiting planets in nearby young clusters offer the opportunity to study the atmospheres and dynamics of planets during their formative years. To this end, we focused on K2-25b -- a close-in ($P$=3.48 days), Neptune-sized exoplanet…

We report the discovery and confirmation of two sub-Saturn planets orbiting a bright (V = 11.3), metal-rich ([Fe/H] = 0.42 $\pm$ 0.04 dex) G3 dwarf in the K2 Campaign 2 field. The planets are 5.68 $\pm$ 0.56 Earth-radii and 7.82 $\pm$ 0.72…

In 2016, Kepler/K2 detected a system of two sub-Neptunes transiting the star HD 224018, one of them showing a mono-transit event. In 2017, we began a spectroscopic follow-up with HARPS-N to measure the dynamical masses of the planets using…

We report the discovery and characterization of three transiting giant planets in the TIC118798035 system. The three planets were identified as transiting candidates from data of the TESS mission, and confirmed with ground-based photometric…

The detection of a super-Earth and three mini-Neptunes transiting the bright ($V$ = 9.2 mag) star HD 108236 (also known as TOI-1233) was recently reported on the basis of TESS and ground-based light curves. We perform a first…

Earth and Planetary Astrophysics · Physics 2021-02-24 A. Bonfanti , L. Delrez , M. J. Hooton , T. G. Wilson , L. Fossati , Y. Alibert , S. Hoyer , A. J. Mustill , H. P. Osborn , V. Adibekyan , D. Gandolfi , S. Salmon , S. G. Sousa , A. Tuson , V. Van Grootel , J. Cabrera , V. Nascimbeni , P. F. L. Maxted , S. C. C. Barros , N. Billot , X. Bonfils , L. Borsato , C. Broeg , M. B. Davies , M. Deleuil , O. D. S. Demangeon , M. Fridlund , G. Lacedelli , M. Lendl , C. Persson , N. C. Santos , G. Scandariato , Gy. M. Szabó , A. Collier Cameron , S. Udry , W. Benz , M. Beck , D. Ehrenreich , A. Fortier , K. G. Isaak , D. Queloz , R. Alonso , J. Asquier , T. Bandy , T. Bárczy , D. Barrado , O. Barragán , W. Baumjohann , T. Beck , A. Bekkelien , M. Bergomi , M-D. Busch , A. Brandeker , V. Cessa , S. Charnoz , B. Chazelas , C. Corral Van Damme , B. -O. Demory , A. Erikson , J. Farinato , D. Futyan , A. Garcia Muñoz , M. Gillon , M. Guedel , P. Guterman , J. Hasiba , K. Heng , E. Hernandez , L. Kiss , T. Kuntzer , J. Laskar , A. Lecavelier des Etangs , C. Lovis , D. Magrin , L. Malvasio , L. Marafatto , H. Michaelis , M. Munari , G. Olofsson , H. Ottacher , R. Ottensamer , I. Pagano , E. Pallé , G. Peter , D. Piazza , G. Piotto , D. Pollacco , R. Ragazzoni , N. Rando , F. Ratti , H. Rauer , I. Ribas , M. Rieder , R. Rohlfs , F. Safa , M. Salatti , D. Ségransan , A. E. Simon , A. M. S. Smith , M. Sordet , M. Steller , N. Thomas , M. Tschentscher , V. Van Eylen , V. Viotto , I. Walter , N. A. Walton , F. Wildi , D. Wolter

We report on the discovery of a transiting Earth-sized (0.95$R_\oplus$) planet around an M3.5 dwarf star at 57$\,$pc, K2-315b. The planet has a period of $\sim$3.14 days, i.e. ${\sim}\pi$, with an instellation of 7.45$\,$S$_{\oplus}$. The…

The detection and characterization of young planetary systems offers a direct path to study the processes that shape planet evolution. We report on the discovery of a sub-Neptune-size planet orbiting the young star HD 110082 (TOI-1098).…

We report the discovery of a Jupiter-size planet transiting a relatively bright (V = 11.56) and metal-rich early K dwarf star with a period of about 2.9 days. On the basis of follow-up photometry and spectroscopy we determine the mass and…

Exoplanets in their infancy are ideal targets to probe the formation and evolution history of planetary systems, including the planet migration and atmospheric evolution and dissipation. In this paper, we present spectroscopic observations…

M dwarf stars are high-priority targets for searches for Earth-size and potentially Earth-like planets, but their planetary systems may form and evolve in very different circumstellar environments than those of solar-type stars. To explore…

We present the discovery and characterization of two warm mini-Neptunes transiting the K3V star TOI-815 in a K-M binary system. Analysis of the spectra and rotation period reveal it to be a young star with an age of $200^{+400}_{-200}$Myr.…

Earth and Planetary Astrophysics · Physics 2024-01-31 Angelica Psaridi , Hugh Osborn , François Bouchy , Monika Lendl , Léna Parc , Nicolas Billot , Christopher Broeg , Sérgio G. Sousa , Vardan Adibekyan , Omar Attia , Andrea Bonfanti , Hritam Chakraborty , Karen A. Collins , Jeanne Davoult , Elisa Delgado-Mena , Nolan Grieves , Tristan Guillot , Alexis Heitzmann , Ravit Helled , Coel Hellier , Jon M. Jenkins , Henrik Knierim , Andreas Krenn , JackJ. Lissauer , Rafael Luque , David Rapetti , Nuno C. Santos , Olga Suárez , Julia Venturini , Francis P. Wilkin , Thomas G. Wilson , Joshua N. Winn , Carl Ziegler , Tiziano Zingales , Yann Alibert , Alexis Brandeker , Jo Ann Egger , Davide Gandolfi , Matthew J. Hooton , Amy Tuson , Solène Ulmer-Moll , Lyu Abe , Romain Allart , Roi Alonso , David R. Anderson , Guillem Anglada , Tamas Bárczy , David Barrado , Susana C. C. Barros , Wolfgang Baumjohann , Mathias Beck , Thomas Beck , Willy Benz , Xavier Bonfils , Luca Borsato , Vincent Bourrier , David R. Ciardi , Andrew Collier Cameron , Sébastien Charnoz , Marion Cointepas , Szilárd Csizmadia , Patricio Cubillos , Gaspare Lo Curto , Melvyn B. Davies , Tansu Daylan , Magali Deleuil , Adrien Deline , Laetitia Delrez , Olivier D. S. Demangeon , Brice-Olivier Demory , Caroline Dorn , Xavier Dumusque , David Ehrenreich , Anders Erikson , Alain Lecavelier des Etangs , Elena Diana de Miguel Ferreras , Andrea Fortier , Luca Fossati , Yolanda G. C. Frensch , Malcolm Fridlund , Michaël Gillon , Manuel Güdel , Maximilian N. Günther , Janis Hagelberg , Christiane Helling , Sergio Hoyer , Kate G. Isaak , Laszlo L. Kiss , Kristine Lam , Jacques Laskar , Baptiste Lavie , Christophe Lovis , Demetrio Magrin , Luca Marafatto , Pierre Maxted , Scott McDermott , Djamel Mékarnia , Christoph Mordasini , Felipe Murgas , Valerio Nascimbeni , Louise D. Nielsen , Göran Olofsson , Roland Ottensamer , Isabella Pagano , Enric Pallé , Gisbert Peter , Giampaolo Piotto , Don Pollacco , Didier Queloz , Roberto Ragazzoni , Devin Ramos , Nicola Rando , Heike Rauer , Christian Reimers , Ignasi Ribas , Sara Seager , Damien Ségransan , Gaetano Scandariato , Attila Simon , Alexis M. S. Smith , Manu Stalport , Manfred Steller , Gyula Szabó , Nicolas Thomas , Tyler A. Pritchard , Stéphane Udry , Carlos Corral Van Damme , Valérie Van Grootel , Eva Villaver , Ingo Walter , Nicholas Walton , Cristilyn N. Watkins , Richard G. West

We report the discovery of two super-Earth mass planets orbiting the nearby K0.5 dwarf HD 7924 which was previously known to host one small planet. The new companions have masses of 7.9 and 6.4 M$_\oplus$, and orbital periods of 15.3 and…

We report the discovery of a compact multi-planet system orbiting the relatively nearby (78pc) and bright ($K=8.9$) K-star, K2-266 (EPIC248435473). We identify up to six possible planets orbiting K2-266 with estimated periods of P$_b$ =…

We present precision radial velocity (RV) data sets from Keck-HIRES and from Lick Observatory's new Automated Planet Finder Telescope and Levy Spectrometer on Mt. Hamilton that reveal a multiple-planet system orbiting the nearby, slightly…

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 two warm sub-Neptunes transiting the bright (G = 9.5 mag) K-dwarf HD 15906 (TOI 461, TIC 4646810). This star was observed by the Transiting Exoplanet Survey Satellite (TESS) in sectors 4 and 31, revealing two…

Earth and Planetary Astrophysics · Physics 2023-06-08 Amy Tuson , Didier Queloz , Hugh P. Osborn , Thomas G. Wilson , Matthew J. Hooton , Mathias Beck , Monika Lendl , Göran Olofsson , Andrea Fortier , Andrea Bonfanti , Alexis Brandeker , Lars A. Buchhave , Andrew Collier Cameron , David R. Ciardi , Karen A. Collins , Davide Gandolfi , Zoltan Garai , Steven Giacalone , João Gomes da Silva , Steve B. Howell , Jayshil A. Patel , Carina M. Persson , Luisa M. Serrano , Sérgio G. Sousa , Solène Ulmer-Moll , Andrew Vanderburg , Carl Ziegler , Yann Alibert , Roi Alonso , Guillem Anglada , Tamas Bárczy , David Barrado Navascues , Susana C. C. Barros , Wolfgang Baumjohann , Thomas Beck , Willy Benz , Nicolas Billot , Xavier Bonfils , Luca Borsato , Christopher Broeg , Juan Cabrera , Sébastien Charnoz , Dennis M. Conti , Szilard Csizmadia , Patricio E. Cubillos , Melvyn B. Davies , Magali Deleuil , Laetitia Delrez , Olivier D. S. Demangeon , Brice-Olivier Demory , Diana Dragomir , Courtney D. Dressing , David Ehrenreich , Anders Erikson , Zahra Essack , Jacopo Farinato , Luca Fossati , Malcolm Fridlund , Elise Furlan , Holden Gill , Michaël Gillon , Crystal L. Gnilka , Erica Gonzales , Manuel Güdel , Maximilian N. Günther , Sergio Hoyer , Kate G. Isaak , Jon M. Jenkins , Laszlo L. Kiss , Jacques Laskar , David W. Latham , Nicholas Law , Alain Lecavelier des Etangs , Gaspare Lo Curto , Christophe Lovis , Rafael Luque , Demetrio Magrin , Andrew W. Mann , Pierre F. L. Maxted , Michel Mayor , Scott McDermott , Marko Mecina , Christoph Mordasini , Annelies Mortier , Valerio Nascimbeni , Roland Ottensamer , Isabella Pagano , Enric Pallé , Gisbert Peter , Giampaolo Piotto , Don Pollacco , Tyler Pritchard , Roberto Ragazzoni , Nicola Rando , Francesco Ratti , Heike Rauer , Ignasi Ribas , George R. Ricker , Martin Rieder , Nuno C. Santos , Arjun B. Savel , Gaetano Scandariato , Richard P. Schwarz , Sara Seager , Damien Ségransan , Avi Shporer , Attila E. Simon , Alexis M. S. Smith , Manfred Steller , Chris Stockdale , Gyula M. Szabó , Nicolas Thomas , Guillermo Torres , René Tronsgaard , Stéphane Udry , Bernd Ulmer , Valérie Van Grootel , Roland Vanderspek , Julia Venturini , Nicholas A. Walton , Joshua N. Winn , Bill Wohler

Multi-planet systems orbiting M dwarfs provide valuable tests of theories of small planet formation and evolution. K2-3 is an early M dwarf hosting three small exoplanets (1.5-2.0 Earth radii) at distances of 0.07-0.20 AU. We measure the…