UCAC4 652-070599 , the SIMBAD biblio

UCAC4 652-070599 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST23:54:09

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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
2016MNRAS.460.3179W viz 16       D               1 77460 19 Distance and extinction determination for APOGEE stars with Bayesian method. WANG J., SHI J., PAN K., 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.
2017MNRAS.466.3344E viz 16       D               1 6111 26 A new method for the asteroseismic determination of the evolutionary state of red-giant stars. ELSWORTH Y., HEKKER S., BASU 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.
2019MNRAS.482..616B viz 16       D               1 6658 8 Coefficients of variation for detecting solar-like oscillations. BELL K.J., HEKKER S. and KUSZLEWICZ J.S.
2018ApJS..239...32P viz 16       D               1 6680 193 The second APOKASC catalog: the empirical approach. PINSONNEAULT M.H., ELSWORTH Y.P., TAYAR J., et al.
2019ApJ...872..137S viz 16       D               1 26099 39 Constraining metallicity-dependent mixing and extra mixing using [C/N] in alpha-rich field giants. SHETRONE M., TAYAR J., JOHNSON J.A., et al.
2019AJ....158..147H viz 16       D               1 44781 43 Spectrophotometric parallaxes with linear models: accurate distances for luminous red-giant stars. HOGG D.W., EILERS A.-C. and RIX H.-W.
2019MNRAS.489.4641E viz 16       D               1 6661 ~ Insights from the APOKASC determination of the evolutionary state of red-giant stars by consolidation of different methods. ELSWORTH Y., HEKKER S., JOHNSON J.A., et al.
2020MNRAS.493.1388Y viz 16       D               1 3215 20 Asteroseismology of luminous red giants with Kepler I: long-period variables with radial and non-radial modes. YU J., BEDDING T.R., STELLO D., et al.
2021AJ....161..100W viz 17       D               1 3212 ~ An intermediate-age alpha-rich Galactic population in K2. WARFIELD J.T., ZINN J.C., PINSONNEAULT M.H., 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.
2021ApJ...912...72M viz 811       D     X         20 32 16 Star formation timescales of the halo populations from asteroseismology and chemical abundances. MATSUNO T., AOKI W., CASAGRANDE L., et al.
2021ApJ...913...11L viz 17       D               1 1901 19 Targeting bright metal-poor stars in the disk and halo systems of the Galaxy. LIMBERG G., SANTUCCI R.M., ROSSI S., et al.
2021A&A...650A.115D viz 17       D               1 2056 6 Seismic constraints on the internal structure of evolved stars: From high-luminosity RGB to AGB stars. DREAU G., MOSSER B., LEBRETON Y., et al.
2022ApJ...926...26S viz 17       D               1 6507 18 Dynamically Tagged Groups of Metal-poor Stars from the Best and Brightest Survey. SHANK D., BEERS T.C., PLACCO V.M., 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.
2022ApJ...929...33H viz 17       D               1 114072 2 Quantifying Chemical and Kinematical Properties of Galactic Disks. HU G. and SHAO Z.
2023A&A...677A..21K viz 17       D               1 18722 ~ Investigating Gaia EDR3 parallax systematics using asteroseismology of Cool Giant Stars observed by Kepler, K2, and TESS I. Asteroseismic distances to 12 500 red-giant stars. KHAN S., MIGLIO A., WILLETT E., et al.

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