UCAC4 659-072124 , the SIMBAD biblio

UCAC4 659-072124 , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST22:06:14


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Title First 3 Authors
2014ApJ...787...47S viz 15       D               1 222 160 A study of the shortest-period planets found with Kepler. SANCHIS-OJEDA R., RAPPAPORT S., WINN J.N., et al.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2017AJ....154..107P viz 16       D               1 1306 226 The California-Kepler Survey. I. High-resolution spectroscopy of 1305 stars hosting Kepler transiting planets. PETIGURA E.A., HOWARD A.W., MARCY G.W., et al.
2017AJ....154..108J viz 16       D               1 3237 137 The California-Kepler Survey. II. Precise physical properties of 2025 Kepler planets and their host stars. JOHNSON J.A., PETIGURA E.A., FULTON B.J., et al.
2019ApJ...875...29M viz 16       D               1 2918 72 A spectroscopic analysis of the California-Kepler Survey sample. I. Stellar parameters, planetary radii, and a slope in the radius gap. MARTINEZ C.F., CUNHA K., GHEZZI L., et al.
2020AJ....160..138H viz 16       D               1 72 17 Ultra-short-period planets are stable against tidal inspiral. HAMER J.H. and SCHLAUFMAN K.C.
2021ApJS..255...17S viz 17       D               1 39591 57 Surface rotation and photometric activity for Kepler targets. II. G and F main-sequence stars and cool subgiant stars. SANTOS A.R.G., BRETON S.N., MATHUR S., et al.
2021AJ....162...98B viz 17       D               1 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., et al.
2022MNRAS.513.2732S 315       D     X C F     6 51 1 fBLS - a fast-folding BLS algorithm. SHAHAF S., ZACKAY B., MAZEH T., et al.
2022A&A...663A...4S viz 17       D               1 14206 7 Assessment of [Fe/H] determinations for FGK stars in spectroscopic surveys. SOUBIRAN C., BROUILLET N. and CASAMIQUELA L.
2024MNRAS.528.4053W 45           X         1 12 ~ The GPU phase folding and deep learning method for detecting exoplanet transits. WANG K., GE J., WILLIS K., et al.
2024AJ....168..109S viz 18       D               2 702 ~ Resonant and Ultra-short-period Planet Systems Are at Opposite Ends of the Exoplanet Age Distribution. SCHMIDT S.P., SCHLAUFMAN K.C. and HAMER J.H.

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