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We present precision 4.5 $\mu$m Spitzer transit photometry of eight planet candidates discovered by the K2 mission: K2-52 b, K2-53 b, EPIC 205084841.01, K2-289 b, K2-174 b, K2-87 b, K2-90 b, and K2-124 b. The sample includes four…

Despite the thousands of planets in orbit around stars known to date, the mechanisms of planetary formation, migration, and atmospheric loss remain unresolved. In this work, we confirm the planetary nature of a young Saturn-size planet…

Theoretical predictions suggest that the distribution of planets in very young stars could be very different to that typically observed in Gyr old systems that are the current focus of radial velocity surveys. However, the detection of…

Solar and Stellar Astrophysics · Physics 2015-06-17 S. V. Jeffers , J. R. Barnes , H. R. A. Jones , A. Reiners , D. J. Pinfield , S. C. Marsden

We describe the discovery of a massive transiting hot Jupiter with a very short orbital period (1.30619 d), which we name TrES-3. From spectroscopy of the host star GSC 03089-00929, we measure T_eff = 5720 +- 150 K, logg=4.6 +- 0.3, and…

We present a catalog of 11 multi-planet systems from Campaigns 1 and 2 of the K2 mission. We report the sizes and orbits of 26 planets split between seven 2-planet systems and four 3-planet systems. These planets stem from a systematic…

We present the discovery and characterization of a new transiting planet from Campaign 17 of the Kepler extended mission K2. HD 119130 b is a warm sub-Neptune on a 17-d orbit around a bright (V = 9.9 mag) solar-like G3 V star with a mass…

We report the discovery of three small transiting planets orbiting GJ 9827, a bright (K = 7.2) nearby late K-type dwarf star. GJ 9827 hosts a $1.62\pm0.11$ $R_{\rm \oplus}$ super Earth on a 1.2 day period, a $1.269^{+0.087}_{-0.089}$…

Young transiting exoplanets (< 100 Myr) provide crucial insight into atmospheric evolution via photoevaporation. However, transmission spectroscopy measurements to determine atmospheric composition and mass loss are challenging due to the…

Context. Low mass stars are currently the best targets for searches for rocky planets in the habitable zone of their host star. Over the last 13 years, precise radial velocities measured with the HARPS spectrograph have identified over a…

Earth and Planetary Astrophysics · Physics 2017-06-23 N. Astudillo-Defru , T. Forveille , X. Bonfils , D. Ségransan , F. Bouchy , X. Delfosse , C. Lovis , M. Mayor , F. Murgas , F. Pepe , N. C. Santos , S. Udry , A. Wunsche

The abundance of planets with orbital periods of a few to tens of days suggests that exoplanets experience complex dynamical histories. Planets in young stellar clusters or associations have well-constrained ages and therefore provide an…

We present the discovery of K2-113b, a dense hot-Jupiter discovered using photometry from Campaign 8 of the Kepler-2 (K2) mission and high-resolution spectroscopic follow up obtained with the FEROS spectrograph. The planet orbits a…

We report on the discovery of three transiting planets around GJ~9827. The planets have radii of 1.75$_{-0.12}^{+0.11 }$, 1.36$_{- 0.09 }^{+ 0.09}$, and 2.10$_{- 0.15 }^{+ 0.15 }$~R$_{\oplus}$, and periods of 1.20896, 3.6480, and 6.2014…

We report the discovery from K2 of a transiting terrestrial planet in an ultra-short-period orbit around an M3-dwarf. K2-137 b completes an orbit in only 4.3 hours, the second-shortest orbital period of any known planet, just 4 minutes…

We present new, high-precision Doppler radial velocity (RV) data sets for the nearby K3V star HD 219134. The data include 175 velocities obtained with the HIRES Spectrograph at the Keck I Telescope, and 101 velocities obtained with the Levy…

TOI-1203 is a bright (V=8.6) G3 V star known to host a transiting warm sub-Neptune on a 25.5 d orbit. Here we report on an intensive high-precision radial velocity and photometric follow-up campaign carried out with the HARPS spectrograph…

Earth and Planetary Astrophysics · Physics 2025-09-15 D. Gandolfi , A. Alnajjarine , L. M. Serrano , J. A. Egger , K. W. F. Lam , J. Cabrera , A. P. Hatzes , M. Fridlund , M. Garbaccio Gili , T. G. Wilson , W. D. Cochran , A. Brandeker , E. Goffo , S. G. Sousa , G. Nowak , A. Heitzmann , C. Hellier , J. Venturini , J. Livingston , A. Bonfanti , O. Barragán , V. Adibekyan , E. Knudstrup , Y. Alibert , S. Grziwa , C. Ziegler , L. Fossati , F. Murgas , A. C. M. Correia , S. H. Albrecht , J. Laskar , E. W. Guenther , S. J. A. J. Salmon , S. Redfield , N. Billot , H. J. Deeg , L. Delrez , L. Palethorpe , V. Van Eylen , F. Rodler , J. Alarcon , J. M. Jenkins , J. D. Twicken , A. W. Mann , R. Alonso , J. Asquier , T. Bárczy , D. Barrado , S. C. C. Barros , W. Baumjohann , W. Benz , L. Borsato , C. Broeg , M. Buder , P. Chaturvedi , A. Collier Cameron , Sz. Csizmadia , P. E. Cubillos , M. B. Davies , M. Deleuil , A. Deline , O. D. S. Demangeon , B. -O. Demory , A. Derekas , B. Edwards , D. Ehrenreich , A. Erikson , A. Fortier , K. Gazeas , M. Gillon , M. Güdel , M. N. Günther , Ch. Helling , K. G. Isaak , L. L. Kiss , J. Korth , N. Law , A. Lecavelier des Etangs , A. Leleu , M. Lendl , P. Leonardi , D. Magrin , G. Mantovan , L. Marafatto , P. F. L. Maxted , M. Mecina , B. Merín , C. Mordasini , V. Nascimbeni , A. Nigioni , G. Olofsson , H. P. Osborn , R. Ottensamer , I. Pagano , E. Pallé , C. M. Persson , G. Peter , D. Piazza , G. Piotto , D. Pollacco , D. Queloz , R. Ragazzoni , N. Rando , H. Rauer , I. Ribas , G. R. Ricker , N. C. Santos , G. Scandariato , S. Seager , D. Ségransan , A. E. Simon , A. M. S. Smith , M. Stalport , S. Sulis , Gy. M. Szabó , S. Udry , S. Ulmer-Moll , V. Van Grootel , E. Villaver , N. A. Walton , J. N. Winn , S. Wolf , T. Zingales

We report the discovery of a brown dwarf companion to the young M dwarf 1RXS J235133.3+312720 as part of a high contrast imaging search for planets around nearby young low-mass stars with Keck-II/NIRC2 and Subaru/HiCIAO. The 2.4" (~120 AU)…

Solar and Stellar Astrophysics · Physics 2015-06-05 Brendan P. Bowler , Michael C. Liu , Evgenya L. Shkolnik , Trent J. Dupuy , Lucas A. Cieza , Adam L. Kraus , Motohide Tamura

Young planets (< 1 Gyr) are helpful for studying the physical processes occurring at the early stage of planet evolution. TOI-251 b is a recently discovered sub-Neptune orbiting a young G dwarf, which has an imprecise age estimation of…

Solar and Stellar Astrophysics · Physics 2023-07-26 Qinghui Sun , Sharon Xuesong Wang , Andrew W. Mann , Benjamin M. Tofflemire , Adam L. Kraus , Tianjun Gan , Madyson G. Barber
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