Hot subluminous stars: Highlights from the MUCHFUSS and Kepler missions by Geier S., Heber U., Gaensicke B.

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Rotation and magnetic activity of oscillating solar-like stars with the Kepler mission by Mathur Savita, Balliet Lauren, García Rafael A., Salabert David

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On Study of the Occurrence of Earth-Size Planets in Kepler Mission Using Spatial Poisson Model by Hong-Ding Yang, Yun-Huan Lee, Che-Yang Lin

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KEPLER-15b: A HOT JUPITER ENRICHED IN HEAVY ELEMENTS AND THE FIRST KEPLER MISSION PLANET CONFIRMED WITH THE HOBBY-EBERLY TELESCOPE by Demory, Brice-Olivier

“…We report the discovery of Kepler-15b (KOI-128), a new transiting exoplanet detected by NASA's Kepler mission. The transit signal with a period of 4.94 days was detected in the quarter 1 (Q1) Kepler photometry. …”
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Highlights of Discoveries for δ Scuti Variable Stars From the Kepler Era by Joyce Ann Guzik

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Revisiting the δ Scuti star FG Virginis using Kepler K2 and TESS data by Joyce A. Guzik, Jason Jackiewicz, Anne M. Hedlund, Anne M. Hedlund

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Properties of 249 δ Scuti Variable Star Candidates Observed During the NASA K2 Mission by Joyce Ann Guzik, Jorge A. Garcia, Jason Jackiewicz

Subjects: “…NASA Kepler mission…”
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The first view of δ Scuti and γ Doradus stars with the TESS mission

“…We derive an empirical estimate of 74 per cent for the relative amplitude suppression factor as a result of the redder TESS passband compared to the Kepler mission using a pulsating eclipsing binary system. …”
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Characteristics of Kepler Planetary Candidates Based on the First Data Set by Seager, Sara

“…On 2010 June 15, the Kepler Mission released most of the data from the first quarter of observations. …”
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The first view of δ Scuti and γ Doradus stars with the TESS mission by Seager, Sara

“…We derive an empirical estimate of 74 per cent for the relative amplitude suppression factor as a result of the redder TESS passband compared to the Kepler mission using a pulsating eclipsing binary system. …”
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Hot Jupiter secondary eclipses measured by Kepler by Seager S., Demory B.-O.

“…The outstanding quality of the Kepler mission photometry allows a detection (or non-detection upper limits on) giant planet secondary eclipses at visible wavelengths. …”
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Reflected eclipses on circumbinary planets by Deeg H.J., Doyle L.R.

“…For the sample of eclipsing binaries found by the Kepler mission, reflected eclipses from close circumbinary planets may be detectable around at least several dozen binaries. …”
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Pulsating white dwarfs by Kepler S.O., Romero Alejandra D.

“…It has also led to the discovery of new types of variable white dwarfs, as the variable hot DQs, and the pulsating Extremely Low Mass white dwarfs. With the Kepler Mission, it has been possible to discover new phenomena, the outbursts present in a few pulsating white dwarfs.…”
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K-band spectroscopic metallicities and temperatures of M-dwarf stars by Rojas-Ayala Bárbara

“…The metallicity distribution of the M dwarf host candidates by the Kepler Mission hints that jovian-size planets form preferentially around solar and super-solar metallicity environments, while small rocky planet host exhibit a wide range of metallicities, just like in their solar-type counterparts.…”
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Old star clusters: Bench tests of low mass stellar models by Salaris M.

“…Moreover, recent results from the Kepler mission about the old open cluster NGC6791 are adding new tight constraints to the models.…”
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The potential of space observations for pulsating pre-main sequence stars by Zwintz Konstanze

“…But it is evident from comparison with the more evolved pulsators in their main sequence or post-main sequence stages observed by the main Kepler mission, that many more questions could be addressed with significantly longer time bases and ultrahigh precision. …”
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Validation and Initial Characterization of the Long-period Planet Kepler-1654 b by Beichman, C. A., Giles, H. A. C., Akeson, R., Ciardi, D., Christiansen, J., Isaacson, H., Marcy, G. M., Sinukoff, E., Greene, T., Fortney, J. J., Hu, R., Howard, A. W., Petigura, E. A., Knutson, H. A., Crossfield, Ian Jm

“…Our early search of the Kepler light curves revealed one such system, Kepler-1654b (originally KIC 8410697b), which shows exactly two transit events and whose second transit occurred only five days before the failure of the second of two reaction wheels brought the primary Kepler mission to an end. A number of authors have also examined light curves from the Kepler mission searching for long-period planets and identified this candidate. …”
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A fitting LEGACY – modelling Kepler's best stars by Aarslev Magnus J., Christensen-Dalsgaard Jørgen, Lund Mikkel N., Aguirre Victor Silva, Gough Douglas

“…The LEGACY sample represents the best solar-like stars observed in the Kepler mission[5, 8]. The 66 stars in the sample are all on the main sequence or only slightly more evolved. …”
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The roAp Stars Observed by the Kepler Space Telescope by Daniel L. Holdsworth

“…Over the duration of the primary 4 year Kepler mission, and its 4 year reconfigured K2 mission, the telescope observed at least 14 new and known roAp stars. …”
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LOW FALSE POSITIVE RATE OF KEPLER CANDIDATES ESTIMATED FROM A COMBINATION OF SPITZER AND FOLLOW-UP OBSERVATIONS by Charbonneau, David, Torres, Guillermo, Fressin, François, Ballard, Sarah, Bryson, Stephen T., Knutson, Heather A., Batalha, Natalie M., Borucki, William J., Brown, Timothy M., Deming, Drake, Ford, Eric B., Fortney, Jonathan J., Gilliland, Ronald L., Latham, David W., Seager, Sara, Desert, Jean-Michel

“…NASA's Kepler mission has provided several thousand transiting planet candidates during the 4 yr of its nominal mission, yet only a small subset of these candidates have been confirmed as true planets. …”
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