KOI-7388 , the SIMBAD biblio

KOI-7388 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST12:43:12

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
2011A&A...529A..89D viz 15       D               1 3298 98 Global stellar variability study in the field-of-view of the Kepler satellite. DEBOSSCHER J., BLOMME J., AERTS C., et al.
2013A&A...560A...4R viz 15       D               1 24132 291 Rotation and differential rotation of active Kepler stars. REINHOLD T., REINERS A. and BASRI G.
2014ApJS..211...24M viz 15       D               1 34022 573 Rotation periods of 34,030 Kepler main-sequence stars: the full autocorrelation sample. McQUILLAN A., MAZEH T. and AIGRAIN S.
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.
2015A&A...583A..65R viz 16       D               1 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
2016ApJ...822...86M viz 16       D               1 6130 337 False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives. MORTON T.D., BRYSON S.T., COUGHLIN J.L., et al.
2016A&A...594A..39F viz 16       D               1 51408 86 Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al.
2019ApJ...871..174S viz 16       D               2 847 5 Rapid rotation in the Kepler field: not a single star phenomenon. SIMONIAN G.V.A., PINSONNEAULT M.H. and TERNDRUP D.M.
2019ApJ...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2019ApJ...884L..42K 16       D               1 12 8 Stars that move together were born together. KAMDAR H., CONROY C., TING Y.-S., et al.
2019ApJS..244...37G viz 16       D               1 1744 ~ Flare activity and magnetic feature analysis of the flare stars. GOODARZI H., MEHRABI A., KHOSROSHAHI H.G., et al.
2020ApJ...888...43C viz 16       D               1 489 32 Chemical evolution in the Milky Way: rotation-based ages for APOGEE-Kepler Cool dwarf stars. CLAYTOR Z.R., VAN SADERS J.L., SANTOS A.R.G., et al.
2020ApJS..247....9Z viz 16       D               1 5575 26 Magnetic activity of F-, G-, and K-type stars in the LAMOST-Kepler field. ZHANG J., BI S., LI Y., et al.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2020MNRAS.499.3481A viz 16       D               1 28505 24 Evidence for metallicity-dependent spin evolution in the Kepler field. AMARD L., ROQUETTE J. and MATT S.P.
2021AJ....161..189L viz 17       D               1 29956 19 Gyro-kinematic ages for around 30,000 Kepler stars. LU Y., ANGUS R., CURTIS J.L., et al.
2021MNRAS.504.5327A 17       D               1 7000 19 Exoplanet validation with machine learning: 50 new validated Kepler planets. ARMSTRONG D.J., GAMPER J. and DAMOULAS T.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2022A&A...664A..78F viz 17       D               1 7452 7 Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al.
2024MNRAS.533.1290S viz 18       D               1 7737 ~ The impact of stellar metallicity on rotation and activity evolution in the Kepler field using gyro-kinematic ages. SEE V., LU Y., AMARD L., et al.

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