2MASS J19283705+3846343 , the SIMBAD biblio

2MASS J19283705+3846343 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST16:48:02


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Title First 3 Authors
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...807...45D viz 16       D               1 2707 726 The occurrence of potentially habitable planets orbiting M dwarfs estimated from the full Kepler dataset and an empirical measurement of the detection sensitivity. DRESSING C.D. and CHARBONNEAU D.
2015A&A...583A..65R viz 16       D               1 20938 134 Rotation, differential rotation, and gyrochronology of active Kepler stars. REINHOLD T. and GIZON L.
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.
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.
2020AJ....160..287S 16       D               5 84 ~ A closer look at exoplanet occurrence rates: considering the multiplicity of stars without detected planets. SAVEL A.B., DRESSING C.D., HIRSCH L.A., et al.
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.
2026AJ....171..110B 20       D               1 41 ~ Modeling the Impact of Unresolved Stellar Companions on Detection Sensitivity in Kepler's Small-planet Occurrence Rates. BERGSTEN G.J., CIARDI D.R., CHRISTIANSEN J.L., et al.

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