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The Kepler K2 mission now makes it possible to find and study a wider variety of eclipsing binary stars than has been possible to-date, particularly long-period systems with narrow eclipses. Our aim is to characterise eclipsing binary stars…

Solar and Stellar Astrophysics · Physics 2018-08-15 P. F. L. Maxted , R. J. Hutcheon

We apply the automated AnomalyFinder algorithm of Paper I (Zang et al. 2021b) to 2018-2019 light curves from the $\simeq 13\,{\rm deg}^2$ covered by the six KMTNet prime fields, with cadences $\Gamma \geq 2\,{\rm hr}^{-1}$. We find a total…

The Transiting Exoplanet Survey Satellite (TESS) is a NASA-sponsored Explorer mission that will perform a wide-field survey for planets that transit bright host stars. Here, we predict the properties of the transiting planets that TESS will…

We present a comprehensive catalog of cool (period $P\gtrsim 2\,\mathrm{yr}$) transiting planet candidates in the four-year light curves from the prime \kepler\ mission. Most of the candidates show only one or two transits and have largely…

Earth and Planetary Astrophysics · Physics 2019-05-15 Hajime Kawahara , Kento Masuda

The number of potentially habitable planets continues to increase, but we lack the time and resources to characterize all of them. With $\sim$30 known potentially habitable planets and an ever-growing number of candidate and confirmed…

Earth and Planetary Astrophysics · Physics 2022-04-27 Austin Ware , Patrick Young , Amanda Truitt , Alexander Spacek

Ranked near the top of the long list of exciting discoveries made with NASA's Kepler photometer is the detection of transiting circumbinary planets. In just over a year the number of such planets went from zero to seven, including a…

Earth and Planetary Astrophysics · Physics 2015-06-17 William F. Welsh , Jerome A. Orosz , Joshua A. Carter , Daniel C. Fabrycky

The Kepler mission found hundreds of planet candidates within the habitable zones (HZ) of their host star, including over 70 candidates with radii larger than 3 Earth radii ($R_\oplus$) within the optimistic habitable zone (OHZ) (Kane et…

Earth and Planetary Astrophysics · Physics 2018-06-21 Michelle L. Hill , Stephen R. Kane , Eduardo Seperuelo Duarte , Ravi K. Kopparapu , Dawn M. Gelino , Robert A. Wittenmyer

We investigated the underlying architecture of planetary systems by deriving the distribution of planet multiplicity (number of planets) and the distribution of orbital inclinations based on the sample of planet candidates discovered by the…

Earth and Planetary Astrophysics · Physics 2015-06-05 Julia Fang , Jean-Luc Margot

The LAMOST-\textit{K}2 (L\textit{K}2) project, initiated in 2015, aims to collect low-resolution spectra of targets in the \textit{K}2 campaigns, similar to LAMOST-\textit{Kepler} project. By the end of 2018, a total of 126 L\textit{K}2…

We present the detection of three super-Earths transiting the cool star LP415-17, monitored by K2 mission in its 13th campaign. High resolution spectra obtained with HARPS-N/TNG showed that the star is a mid-late K dwarf. Using spectral…

We report the results of an observational study aimed at searching for magnetic pulsating hot stars suitable for magneto-asteroseismology. A sample of sixteen chemically peculiar stars was selected and analysed using both high-resolution…

Solar and Stellar Astrophysics · Physics 2018-07-04 B. Buysschaert , C. Neiner , A. J. Martin , C. Aerts , D. M. Bowman , M. E. Oksala , T. Van Reeth

The NASA K2 mission that succeeded the nominal Kepler mission observed several hundreds of thousands of stars during its operations. While most of the stars were observed in single campaigns of 80 days, some of them were targeted for more…

The Transiting Exoplanet Survey Satellite (TESS) has discovered hundreds of new worlds, with TESS planet candidates now outnumbering the total number of confirmed planets from $\textit{Kepler}$. Owing to differences in survey design, TESS…

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…

We present robust planet occurrence rates for Kepler planet candidates around M stars for planet radii $R_p = 0.5-4~\textrm{R}_\oplus$ and orbital periods $P = 0.5-256$ days using the approximate Bayesian computation (ABC) technique. This…

Earth and Planetary Astrophysics · Physics 2020-09-09 Danley C. Hsu , Eric B. Ford , Ryan Terrien

PLATO 2.0 has recently been selected for ESA's M3 launch opportunity (2022/24). Providing accurate key planet parameters (radius, mass, density and age) in statistical numbers, it addresses fundamental questions such as: How do planetary…

Earth and Planetary Astrophysics · Physics 2015-06-17 H. Rauer , C. Catala , C. Aerts , T. Appourchaux , W. Benz , A. Brandeker , J. Christensen-Dalsgaard , M. Deleuil , L. Gizon , M. -J. Goupil , M. Güdel , E. Janot-Pacheco , M. Mas-Hesse , I. Pagano , G. Piotto , D. Pollacco , N. C. Santos , A. Smith , J. -C. , Suárez , R. Szabó , S. Udry , V. Adibekyan , Y. Alibert , J. -M. Almenara , P. Amaro-Seoane , M. Ammler-von Eiff , M. Asplund , E. Antonello , W. Ball , S. Barnes , F. Baudin , K. Belkacem , M. Bergemann , G. Bihain , A. C. Birch , X. Bonfils , I. Boisse , A. S. Bonomo , F. Borsa , I. M. Brandão , E. Brocato , S. Brun , M. Burleigh , R. Burston , J. Cabrera , S. Cassisi , W. Chaplin , S. Charpinet , C. Chiappini , R. P. Church , Sz. Csizmadia , M. Cunha , M. Damasso , M. B. Davies , H. J. Deeg , R. F. DÍaz , S. Dreizler , C. Dreyer , P. Eggenberger , D. Ehrenreich , P. Eigmüller , A. Erikson , R. Farmer , S. Feltzing , F. de Oliveira Fialho , P. Figueira , T. Forveille , M. Fridlund , R. A. García , P. Giommi , G. Giuffrida , M. Godolt , J. Gomes da Silva , T. Granzer , J. L. Grenfell , A. Grotsch-Noels , E. Günther , C. A. Haswell , A. P. Hatzes , G. Hébrard , S. Hekker , R. Helled , K. Heng , J. M. Jenkins , A. Johansen , M. L. Khodachenko , K. G. Kislyakova , W. Kley , U. Kolb , N. Krivova , F. Kupka , H. Lammer , A. F. Lanza , Y. Lebreton , D. Magrin , P. Marcos-Arenal , P. M. Marrese , J. P. Marques , J. Martins , S. Mathis , S. Mathur , S. Messina , A. Miglio , J. Montalban , M. Montalto , M. J. P. F. G. Monteiro , H. Moradi , E. Moravveji , C. Mordasini , T. Morel , A. Mortier , V. Nascimbeni , R. P. Nelson , M. B. Nielsen , L. Noack , A. J. Norton , A. Ofir , M. Oshagh , R. -M. Ouazzani , P. Pápics , V. C. Parro , P. Petit , B. Plez , E. Poretti , A. Quirrenbach , R. Ragazzoni , G. Raimondo , M. Rainer , D. R. Reese , R. Redmer , S. Reffert , B. Rojas-Ayala , I. W. Roxburgh , S. Salmon , A. Santerne , J. Schneider , J. Schou , S. Schuh , H. Schunker , A. Silva-Valio , R. Silvotti , I. Skillen , I. Snellen , F. Sohl , S. G. Sousa , A. Sozzetti , D. Stello , K. G. Strassmeier , M. Švanda , Gy. M. Szabó , A. Tkachenko , D. Valencia , V. van Grootel , S. D. Vauclair , P. Ventura , F. W. Wagner , N. A. Walton , J. Weingrill , S. C. Werner , P. J. Wheatley , K. Zwintz

A commissioning survey of the Lookout Observatory has observed fourteen faint (V ~ 13 to 17) variables in the region of the exoplanet Kepler-8b. Three of these are variable star candidates discovered by the Asteroid Terrestrial-Impact Last…

Solar and Stellar Astrophysics · Physics 2020-12-22 Neil Thomas , Margaret Paczkowski

NASA's Kepler Space Telescope has collected high-precision, high-cadence time series photometry on 781,590 unique postage-stamp targets across 21 different fields of view. These observations have already yielded 2,496 scientific…

Results from the Kepler mission indicate that the occurrence rate of small planets ($<3$ $R_\oplus$) in the habitable zone of nearby low-mass stars may be as high as 80%. Despite this abundance, probing the conditions and atmospheric…

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