2MASS J19235436+3740359 , the SIMBAD biblio

2MASS J19235436+3740359 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.16CEST13:57:31

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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
2014A&A...572L...5M viz 16       D               1 1210 165 Mixed modes in red giants: a window on stellar evolution. MOSSER B., BENOMAR O., BELKACEM K., 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.
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.
2017MNRAS.469.4578H viz 16       D               1 8666 48 Deep learning classification in asteroseismology. 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...618A.109M viz 16       D               1 397 53 Period spacings in red giants. IV. Toward a complete description of the mixed-mode pattern. MOSSER B., GEHAN C., BELKACEM K., et al.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2020AJ....160..120J viz 17       D               1 365761 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.
2020ApJ...900....4S viz 17       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.
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.

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