BD+41 3257C , the SIMBAD biblio

BD+41 3257C , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST09:34:00

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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
2013A&A...553A.127P viz 39           X         1 5 18 Two new SB2 binaries with main sequence B-type pulsators in the Kepler field. PAPICS P.I., TKACHENKO A., AERTS C., et al.
2016A&A...588A..87V viz 16       D               1 6115 133 Period spacings in red giants. II. Automated measurement. VRARD M., MOSSER B. and SAMADI R.
2016AJ....152....6W viz 16       D               1 3060 13 Calibration of LAMOST stellar surface gravities using the Kepler asteroseismic data. WANG L., WANG W., WU Y., 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.
2017A&A...600A...1M viz 16       D               1 5166 19 Period spacings in red giants. III. Coupling factors of mixed modes. MOSSER B., PINCON C., BELKACEM K., et al.
2018MNRAS.475.3633W viz 16       D               1 3727 38 Mass and age of red giant branch stars observed with LAMOST and Kepler. WU Y., XIANG M., BI S., et al.
2018MNRAS.476.3233H viz 16       D               1 15009 17 Deep learning classification in asteroseismology using an improved neural network: results on 15 000 Kepler red giants and applications to K2 and TESS data. HON M., STELLO D. and YU J.
2018ApJS..236...42Y viz 16       D               1 16097 158 Asteroseismology of 16,000 Kepler red giants: global oscillation parameters, masses, and radii. YU J., HUBER D., BEDDING T.R., et al.
2018A&A...616A..24G viz 16       D               1 1140 108 Core rotation braking on the red giant branch for various mass ranges. GEHAN C., MOSSER B., MICHEL E., et al.
2019MNRAS.488..572K viz 16       D               2 95 ~ Bayesian hierarchical inference of asteroseismic inclination angles. KUSZLEWICZ J.S., CHAPLIN W.J., NORTH T.S.H., et al.
2020A&A...639A..63G viz 16       D               1 4575 22 Active red giants: Close binaries versus single rapid rotators. GAULME P., JACKIEWICZ J., SPADA F., et al.
2020ApJS..251...15Z viz 16       D               1 20886 38 Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. ZONG W., FU J.-N., DE CAT P., et al.
2021A&A...645A.124G viz 17       D               2 1202 13 Automated approach to measure stellar inclinations: validation through large-scale measurements on the red giant branch. GEHAN C., MOSSER B., MICHEL E., et al.
2021AJ....161..170S viz 17       D               1 16187 ~ The Swan: data-driven inference of stellar surface gravities for cool stars from photometric light curves. SAYEED M., HUBER D., WHEELER A., et al.
2022ApJ...927..167L viz 17       D               1 3663 12 Asteroseismology of 3642 Kepler Red Giants: Correcting the Scaling Relations Based on Detailed Modeling. LI T., LI Y., BI S., 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.
2023ApJ...944L...5M viz 17       D               1 1240 3 Lithium Abundances in Giants as a Function of Stellar Mass: Evidence for He Flash as the Source of Li Enhancement in Low-mass Giants. MALLICK A., SINGH R. and REDDY B.E.
2023ApJ...953..182W viz 17       D               1 1158 ~ Asteroseismic Modeling of 1153 Kepler Red Giant Branch Stars: Improved Stellar Parameters with Gravity-mode Period Spacings and Luminosity Constraints. WANG Y., LI T., BI S., et al.
2023ApJ...954..152K viz 17       D               1 1077 ~ Mixed-mode Ensemble Asteroseismology of Low-luminosity Kepler Red Giants. KUSZLEWICZ J.S., HON M. and HUBER D.
2024A&A...686A..93G viz 18       D               1 4574 ~ Magnetic activity of red giants: Correlation between the amplitude of solar-like oscillations and chromospheric indicators. GEHAN C., GODOY-RIVERA D. and GAULME P.

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