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Related papers: M2K: II. A Triple-Planet System Orbiting HIP 57274

200 papers

$K2$ greatly extended $Kepler$'s ability to find new planets, but it was typically limited to identifying transiting planets with orbital periods below 40 days. While analyzing $K2$ data through the Exoplanet Explorers project, citizen…

We have found a system listed in the Kepler Binary Catalog (3.273 day period; Prsa et al. 2010) that we have determined is comprised of a low-mass, thermally-bloated, hot white dwarf orbiting an A star of about 2.3 solar masses. In this…

Solar and Stellar Astrophysics · Physics 2015-05-20 Joshua A. Carter , Saul Rappaport , Daniel Fabrycky

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…

We report the discovery and initial characterization of Qatar-2b, a hot Jupiter transiting a V = 13.3 mag K dwarf in a circular orbit with a short period, P_ b = 1.34 days. The mass and radius of Qatar-2b are M_p = 2.49 M_j and R_p = 1.14…

In this paper, we report the evidence for a planetary mass body orbiting the close binary star KIC 5095269. This detection arose from a search for eclipse timing variations among the more than 2,000 eclipsing binaries observed by Kepler.…

Earth and Planetary Astrophysics · Physics 2017-05-03 A. K. Getley , B. Carter , R. King , S. O'Toole

We present an intensive effort to refine the mass and orbit of the enveloped terrestrial planet GJ 1214 b using 165 radial velocity (RV) measurements taken with the HARPS spectrograph over a period of ten years. We conduct a joint analysis…

Earth and Planetary Astrophysics · Physics 2021-10-13 Ryan Cloutier , David Charbonneau , Drake Deming , Xavier Bonfils , Nicola Astudillo-Defru

We report the discovery of a multi-planet system orbiting HD 106315, a rapidly rotating mid F-type star, using data from the K2 mission. HD 106315 hosts a $2.51\pm0.12\,R_\oplus$ sub-Neptune in a 9.5 day orbit, and a…

We report the discovery and characterisation of the multi-planetary system around TOI-4311, a K dwarf kinematically between the Galactic thick disk and Hercules stream. TOI-4311 hosts an ultra-short-period super-Earth (P$\sim$0.99 d,…

Earth and Planetary Astrophysics · Physics 2026-05-13 Yoshi Nike Emilia Eschen , Thomas G. Wilson , Andrew Collier Cameron , Alexander James Mustill , Jo Ann Egger , Solène Ulmer-Moll , Davide Gandolfi , Alexis M. S. Smith , Olivier D. S. Demangeon , Sérgio G. Sousa , Andrea Bonfanti , Alexandre C. M. Correia , Vardan Adibekyan , Gaia Lacedelli , Alexis Brandeker , Camilla Pezzotti , Babatunde Akinsanmi , Yann Alibert , Roi Alonso , Tamas Bárczy , David Barrado , Susana C. C. Barros , Wolfgang Baumjohann , Willy Benz , Nicolas Billot , Luca Borsato , Christopher Broeg , Amadeo Castro-González , Szilard Csizmadia , Patricio E. Cubillos , Melvyn B. Davies , Magali Deleuil , Adrien Deline , Brice-Olivier Demory , Aliz Derekas , Giuseppe Di Persio , Billy Edwards , David Ehrenreich , Anders Erikson , Andrea Fortier , Luca Fossati , Malcolm Fridlund , Kosmas Gazeas , Michaël Gillon , Manuel Güdel , Maximilian N. Günther , Alexis Heitzmann , Ch. Helling , Kate G. Isaak , Jon M. Jenkins , Tatiana Keller , Laszlo L. Kiss , Daniel Kitzmann , Judith Korth , Kristine W. F. Lam , Jacques Laskar , Alain Lecavelier des Etangs , Adrien Leleu , Monika Lendl , Demetrio Magrin , Pierre F. L. Maxted , Bruno Merín , Christoph Mordasini , Valerio Nascimbeni , Göran Olofsson , Hugh P. Osborn , Roland Ottensamer , Isabella Pagano , Enric Pallé , Gisbert Peter , Glen Petitpas , Daniele Piazza , Giampaolo Piotto , Don Pollacco , Didier Queloz , Roberto Ragazzoni , Nicola Rando , Heike Rauer , Ignasi Ribas , Nuno C. Santos , Gaetano Scandariato , Damien Ségransan , Avi Shporer , André M. Silva , Attila E. Simon , Richard Southworth , Manu Stalport , Sophia Sulis , Gyula M. Szabó , Stéphane Udry , Bernd Ulmer , Valérie Van Grootel , Julia Venturini , Eva Villaver , Nicholas A. Walton , Sebastian Wolf , Carl Ziegler , Tiziano Zingales

Transiting exoplanets in young open clusters present opportunities to study how exoplanets evolve over their lifetimes. Recently, significant progress detecting transiting planets in young open clusters has been made with the K2 mission,…

This paper reports on the detection of two new multiple planet systems around solar-like stars HD47186 and HD181433. The first system includes a hot Neptune of 22.78 M_Earth at 4.08-days period and a Saturn of 0.35 M_Jup at 3.7-years…

Initially designed to discover short-period planets, the N2K campaign has since evolved to discover new worlds at large separations from their host stars. Detecting such worlds will help determine the giant planet occurrence at semi-major…

We have studied the possibility that a third circumbinary planet in the Kepler-47 planetary system be the source of the single unexplained transiting event reported during the discovery of these planets. We applied the MEGNO technique to…

Earth and Planetary Astrophysics · Physics 2015-06-22 Tobias C. Hinse , Nader Haghighipour , Veselin B. Kostov , Krzysztof Goździewski

Spectroscopic orbits are computed for inner pairs in 9 hierarchical multiple systems (HIP 19639, 60845, 75663, 76816, 78163, 78416, 80448, 84789, and HD 105080) and for one simple binary HIP 61840. All subsystems are double-lined, and their…

Solar and Stellar Astrophysics · Physics 2018-10-24 Andrei Tokovinin

We report on Doppler observations of three transiting planet candidates that were detected during Campaign 1 of the K2 mission. The Doppler observations were conducted with FIES, HARPS-N and HARPS. We measure the mass of K2-27b (EPIC…

This work extends the still modest number of multiple stars with known relative orbit orientation. Accurate astrometry and radial velocities are used jointly to compute or update outer and inner orbits in three nearby triple systems HIP…

Solar and Stellar Astrophysics · Physics 2017-04-19 Andrei Tokovinin , David W. Latham

Context: How planet properties depend on stellar mass is a key diagnostic of planetary formation mechanisms. Aims: This motivates planet searches around stars which are significantly more massive or less massive than the Sun, and in…

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