UCAC4 651-075375 , the SIMBAD biblio

UCAC4 651-075375 , the SIMBAD biblio (31 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST18:17:54


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Title First 3 Authors
2010ApJ...713L.182S 17       D               2 13 77 Detection of solar-like oscillations from Kepler photometry of the open cluster NGC 6819. STELLO D., BASU S., BRUNTT H., et al.
2011ApJ...739...13S 41           X         1 14 96 An asteroseismic membership study of the red giants in three open clusters observed by Kepler: NGC 6791, NGC 6819, and NGC 6811. STELLO D., MEIBOM S., GILLILAND R.L., et al.
2013ApJ...767L..19A 77           X         2 12 21 A lithium-rich red giant below the clump in the Kepler cluster, NGC 6819. ANTHONY-TWAROG B.J., DELIYANNIS C.P., RICH E., et al.
2014ApJ...787..110C viz 15       D               1 996 100 Stromgren survey for Asteroseismology and Galactic Archaeology: let the SAGA begin. CASAGRANDE L., SILVA AGUIRRE V., STELLO D., et al.
2014AJ....148...38M viz 15       D               1 2648 65 WIYN open cluster study. LX. Spectroscopic binary orbits in NGC 6819. MILLIMAN K.E., MATHIEU R.D., GELLER A.M., et al.
2015AJ....149..121L viz 16       D               1 338 16 Spectroscopic abundances in the open cluster NGC 6819. LEE-BROWN D.B., ANTHONY-TWAROG B.J., DELIYANNIS C.P., et al.
2015RAA....15.1197Z viz 16       D               1 1903 4 Candidate members of star clusters from LAMOST DR2. ZHANG B., CHEN X.-Y., LIU C., et al.
2015RAA....15.2193G viz 16       D               1 539 3 3D cluster members and near-infrared distance of open cluster NGC 6819. GAO X.-H., XU S.-K. and CHEN L.
2016ApJ...823..114N viz 16       D               1 72935 173 Spectroscopic determination of masses (and implied ages) for red giants. NESS M., HOGG D.W., RIX H.-W., et al.
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.
2018AJ....156...18P viz 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 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.
2018AJ....156..142D viz 16       D               2 1381 47 The Open Cluster Chemical Abundances and Mapping survey. II. Precision cluster abundances for APOGEE using SDSS DR14. DONOR J., FRINCHABOY P.M., CUNHA K., 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...879...69T viz 16       D               1 222610 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., 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.
2019AJ....158..163D viz 16       D               1 357 ~ Li evolution and the open cluster NGC 6819: a correlation between Li depletion and spindown in dwarfs more massive than the F-dwarf Li-dip. DELIYANNIS C.P., ANTHONY-TWAROG B.J., LEE-BROWN D.B., et al.
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.
2020AJ....160..120J viz 16       D               1 365763 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 16       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.
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.
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.
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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