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UCAC4 652-080916 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.05.19CEST16:30:23 |
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 | 16 | D | 1 | 6115 | 133 | Period spacings in red giants. II. Automated measurement. | VRARD M., MOSSER B. and SAMADI R. | ||
2017A&A...600A...1M | 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.476.3233H | 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. | ||
2018AJ....156...18P | 16 | D | 1 | 51824 | 872 | Binary companions of evolved stars in APOGEE DR14: search method and catalog of ∼5000 companions. | PRICE-WHELAN A.M., HOGG D.W., RIX H.-W., et al. | ||
2018ApJS..236...42Y | 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. | ||
2019ApJ...878...21T | 17 | D | 1 | 20765 | 54 | The vertical motion history of disk stars throughout the Galaxy. | TING Y.-S. and RIX H.-W. | ||
2019ApJ...879...69T | 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 | 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 | 17 | D | 1 | 121537 | 14 | The age distribution of stars in the Milky Way bulge. | SIT T. and NESS M.K. | ||
2021AJ....161..170S | 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. |