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Rotation periods, variability properties and ages for Kepler exoplanet candidate host stars

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FAST RISE OF “NEPTUNE-SIZE” PLANETS (4-8R⊕) FROMP∼ 10 TO ∼250 DAYS—STATISTICS OFKEPLERPLANET CANDIDATES UP TO ∼0.75 AU

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CoRoT 101186644: A transiting low-mass dense M-dwarf on an eccentric 20.7-day period orbit around a late F-star

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SPECTROSCOPY OF FAINTKEPLERMISSION EXOPLANET CANDIDATE HOST STARS

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THE HUNT FOR EXOMOONS WITH KEPLER (HEK). II. ANALYSIS OF SEVEN VIABLE SATELLITE-HOSTING PLANET CANDIDATES

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ON THE RELATIVE SIZES OF PLANETS WITHINKEPLERMULTIPLE-CANDIDATE SYSTEMS

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The contribution of secondary eclipses as astrophysical false positives to exoplanet transit surveys

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TRANSIT TIMING OBSERVATIONS FROM KEPLER . VIII. CATALOG OF TRANSIT TIMING MEASUREMENTS OF THE FIRST TWELVE QUARTERS

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