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We present two new planetary systems found around cool dwarf stars with data from the K2 mission. The first system was found in K2-239 (EPIC 248545986), char- acterized in this work as M3.0V and observed in the 14th campaign of K2. It…

Small, cool planets represent the typical end-products of planetary formation. Studying the archi- tectures of these systems, measuring planet masses and radii, and observing these planets' atmospheres during transit directly informs…

We report on the discovery of three transiting super-Earths around K2-155 (EPIC 210897587), a relatively bright early M dwarf ($V=12.81$ mag) observed during Campaign 13 of the NASA K2 mission. To characterize the system and validate the…

The TRAPPIST-1 system is the first transiting planet system found orbiting an ultra-cool dwarf star. At least seven planets similar to Earth in radius and in mass were previously found to transit this host star. Subsequently, TRAPPIST-1 was…

We report on the detection of three transiting small planets around the low-mass star LP 358-499 (K2-133), using photometric data from the Kepler-K2 mission. Using multiband photometry, we determine the host star to be an early M dwarf with…

Earth and Planetary Astrophysics · Physics 2017-10-17 R. Wells , K. Poppenhaeger , C. A. Watson

We present a super-Earth orbiting close to the inner edge of the habitable zone of the cool dwarf star K2-286 (EPIC 249889081), detected with data from the K2 mission in its $15^{th}$ campaign. The planet has radius of $2.1\pm0.2$…

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…

We report the detection of three small transiting planets around the young K3 dwarf K2-233 (2MASS J15215519-2013539) from observations during Campaign 15 of the K2 mission. The star is relatively nearby ($d$ = 69 pc) and bright ($V$ = 10.7…

We present moderate resolution near-infrared spectra in $H, J$ and $K$ band of M dwarf hosts to candidate transiting exoplanets discovered by NASA's K2 mission. We employ known empirical relationships between spectral features and physical…

Star-like objects with effective temperatures of less than 2,700 kelvin are referred to as ultracool dwarfs. This heterogeneous group includes stars of extremely low mass as well as brown dwarfs (substellar objects not massive enough to…

The NASA K2 mission uses photometry to find planets transiting stars of various types. M dwarfs are of high interest since they host more short period planets than any other type of main sequence stars and transiting planets around M dwarfs…

Discoveries from the prime Kepler mission demonstrated that small planets (< 3 Earth-radii) are common outcomes of planet formation. While Kepler detected many such planets, all but a handful orbit faint, distant stars and are not amenable…

The nearest exoplanets to the Sun are our best possibilities for detailed characterization. We report the discovery of a compact multi-planet system of super-Earths orbiting the nearby red dwarf GJ 887, using radial velocity measurements.…

This paper reports on the detection of a planetary system with three Super-Earths orbiting HD40307. HD40307 is a K2V metal-deficient star at a distance of only 13 parsec, part of the HARPS GTO high-precision planet-search programme. The…

Astrophysics · Physics 2009-11-13 M. Mayor , S. Udry , C. Lovis , F. Pepe , D. Queloz , W. Benz , J. -L. Bertaux , F. Bouchy , C. Mordasini , D. Segransan

Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary population largely unexplored, and only one of them,…

Earth and Planetary Astrophysics · Physics 2024-06-04 Michaël Gillon , Peter P. Pedersen , Benjamin V. Rackham , Georgina Dransfield , Elsa Ducrot , Khalid Barkaoui , Artem Y. Burdanov , Urs Schroffenegger , Yilen Gómez Maqueo Chew , Susan M. Lederer , Roi Alonso , Adam J. Burgasser , Steve B. Howell , Norio Narita , Julien de Wit , Brice-Olivier Demory , Didier Queloz , Amaury H. M. J. Triaud , Laetitia Delrez , Emmanuël Jehin , Matthew J. Hooton , Lionel J. Garcia , Clàudia Jano Muñoz , Catriona A. Murray , Francisco J. Pozuelos , Daniel Sebastian , Mathilde Timmermans , Samantha J. Thompson , Sebastián Zúñiga-Fernández 1 , Jesús Aceituno , Christian Aganze , Pedro J. Amado , Thomas Baycroft , Zouhair Benkhaldoun , David Berardo , Emeline Bolmont , Catherine A. Clark , Yasmin T. Davis , Fatemeh Davoudi , Zoë L. de Beurs , Jerome P. de Leon , Masahiro Ikoma , Kai Ikuta , Keisuke Isogai , Izuru Fukuda , Akihiko Fukui , Roman Gerasimov , Mourad Ghachoui , Maximilian N. Günther , Samantha Hasler , Yuya Hayashi , Kevin Heng , Renyu Hu , Taiki Kagetani , Yugo Kawai , Kiyoe Kawauchi , Daniel Kitzmann , Daniel D. B. Koll , Monika Lendl , John H. Livingston , Xintong Lyu , Erik A. Meier Valdés , Mayuko Mori , James J. McCormac , Felipe Murgas , Prajwal Niraula , Enric Pallé , Ilse Plauchu-Frayn , Rafael Rebolo , Laurence Sabin , Yannick Schackey , Nicole Schanche , Franck Selsis , Alfredo Sota , Manu Stalport , Matthew R. Standing , Keivan G. Stassun , Motohide Tamura , Christopher A. Theissen , Martin Turbet , Valérie Van Grootel , Roberto Varas , Noriharu Watanabe , Francis Zong Lang

We report the discovery of two transiting planets orbiting K2-290 (EPIC 249624646), a bright (V=11.11) late F-type star residing in a triple-star system. It was observed during Campaign 15 of the K2 mission, and in order to confirm and…

M dwarf stars, which have masses less than 60 per cent that of the Sun, make up 75 per cent of the population of the stars in the Galaxy [1]. The atmospheres of orbiting Earth-sized planets are observationally accessible via transmission…

We report the discovery of two super-Earth-sized planets transiting the bright (V = 8.94, K = 7.07) nearby late G-dwarf HD 3167, using data collected by the K2 mission. The inner planet, HD 3167 b, has a radius of 1.6 R_e and an ultra-short…

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