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The transit method is currently one of our best means for the detection of potentially habitable "Earth-like" exoplanets. In principle, given sufficiently high photometric precision, cool Earth-sized exoplanets orbiting Sun-like stars could…

We have analyzed data from Campaigns 0-5 of the K2 mission and report 19 ultra-short-period candidate planets with orbital periods of less than 1 day (nine of which have not been previously reported). Planet candidates range in size from…

Earth and Planetary Astrophysics · Physics 2016-08-17 Elisabeth R. Adams , Brian Jackson , Michael Endl

Fewer than 20 transiting Kepler planets have periods longer than one year. Our early search of the Kepler light curves revealed one such system, Kepler-1654 b (originally KIC~8410697b), which shows exactly two transit events and whose…

We present 44 days of high duty cycle, ultra precise photometry of the 13th magnitude star Kepler-5 (KIC 8191672, Teff=6300 K, logg=4.1), which exhibits periodic transits with a depth of 0.7%. Detailed modeling of the transit is consistent…

We report on the discovery of K2-141 b (EPIC 246393474 b), an ultra-short-period super-Earth on a 6.7-hour orbit transiting an active K7 V star based on data from K2 campaign 12. We confirmed the planet's existence and measured its mass…

We report the discovery of EPIC201702477b, a transiting brown dwarf in a long period (40.73691 +/- 0.00037 day) and eccentric (e=0.2281 +/- 0.0026) orbit. This system was initially reported as a planetary candidate based on two transit…

Photometric surveys such as Kepler have the precision to identify exoplanet and eclipsing binary candidates from only a single transit. K2, with its 75d campaign duration, is ideally suited to detect significant numbers of single-eclipsing…

We report on the discovery and characterization of the transiting planet K2-39b (EPIC 206247743b). With an orbital period of 4.6 days, it is the shortest-period planet orbiting a subgiant star known to date. Such planets are rare, with only…

Early time-series photometry from NASA's Kepler spacecraft has revealed a planet transiting the star we term Kepler-4, at RA = 19h02m27.68s, Dec = +50:08:08.7. The planet has an orbital period of 3.213 days and shows transits with a…

A search of the time-series photometry from NASA's Kepler spacecraft reveals a transiting planet candidate orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days. The characteristics of the host star are well…

Earth and Planetary Astrophysics · Physics 2015-06-03 William J. Borucki , David G. Koch , Natalie Batalha , Stephen T. Bryson , Douglas A. Caldwell , Jørgen Christensen-Dalsgaard , William D. Cochran , Edna DeVore , Thomas N. Gautier , John C. Geary , Ronald Gilliland , Alan Gould , Steve B. Howell , Jon M. Jenkins , David W. Latham , Jack J. Lissauer , Geoffrey W. Marcy , Jason Rowe , Dimitar Sasselov , Alan Boss , David Charbonneau , David Ciardi , Guillermo Torres , Francois Fressin , Lisa Kaltenegger , Laurance Doyle , Andrea K. Dupree , Eric B. Ford , Jonathan Fortney , Matthew J. Holman , Jason A. Steffen , Fergal Mullally , Martin Still , Jill Tarter , Sarah Ballard , Lars A. Buchhave , Josh Carter , Jessie L. Christiansen , Brice-Olivier Demory , Jean-Michel Désert , Courtney Dressing , Michael Endl , Daniel Fabrycky , Debra Fischer , Michael R. Haas , Christopher Henze , Elliott Horch , Andrew W. Howard , Howard Isaacson , Hans Kjeldsen , John Asher Johnson , Todd Klaus , Jeffery Kolodziejczak , Thomas Barclay , Jie Li , Søren Meibom , Andrej Prsa , Samuel N. Quinn , Elisa V. Quintana , Paul Robertson , William Sherry , Avi Shporer , Peter Tenenbaum , Susan E. Thompson , Joseph D. Twicken , Jeffrey Van Cleve , William F. Welsh , Sarbani Basu , Bill Chaplin , Andrea Miglio , Steve Kawaler , Torben Arentoft , Dennis Stello , Travis S. Metcalfe , Graham Verner , Christoffer Karoff , Mia Lundkvist , Mikkel Lund , Rasmus Handberg , Yvonne Elsworth , Saskia Hekker , Daniel Huber , Timothy R. Bedding

We report the first results from a search for transiting warm Jupiter exoplanets - gas giant planets receiving stellar irradiation below about $10^8$ erg s$^{-1}$ cm$^{-2}$, equivalent to orbital periods beyond about 10 days around Sun-like…

This paper reports on the validation and mass measurement of K2-263b, a sub-Neptune orbiting a quiet G9V star. Using K2 data from campaigns C5 and C16, we find this planet to have a period of $50.818947\pm 0.000094$ days and a radius of…

We confirm the planetary nature of two transiting hot Jupiters discovered by the Kepler spacecraft's K2 extended mission in its Campaign 4, using precise radial velocity measurements from FIES@NOT, HARPS-N@TNG, and the coud\'e spectrograph…

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 report the detection of a single transit-like signal in the Kepler data of the slightly evolved F star KIC4918810. The transit duration is ~45 hours, and while the orbital period ($P\sim10$ years) is not well constrained, it is one of…

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…

We present the discovery of a transiting exoplanet candidate in the K2 Field-1 with an orbital period of 9.1457 hr: K2-22b. The highly variable transit depths, ranging from $\sim$0\% to 1.3\%, are suggestive of a planet that is…

We report on the discovery and validation of Kepler-452b, a transiting planet identified by a search through the 4 years of data collected by NASA's Kepler Mission. This possibly rocky 1.63$^{+0.23}_{-0.20}$ R$_\oplus$ planet orbits its G2…

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…

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