2MASS J19020408+4742298 , the SIMBAD biblio

2MASS J19020408+4742298 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST12:36:41


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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
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.
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.
2021A&A...645A.124G viz 17       D               1 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.

goto View the references in ADS