CoRoT 102686562 , the SIMBAD biblio

CoRoT 102686562 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST12:23:19


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Title First 3 Authors
2012A&A...543A.125G viz 15       D               1 8514 16 Multi-object spectroscopy of stars in the CoRoT fields. II. The stellar population of the CoRoT fields IRa01, LRa01, LRa02, and LRa06. GUENTHER E.W., GANDOLFI D., SEBASTIAN D., et al.
2013A&A...550A.120S viz 16       D               1 6832 13 Improved variability classification of CoRoT targets with Giraffe spectra. SARRO L.M., DEBOSSCHER J., NEINER C., et al.
2016ApJ...823..114N viz 16       D               2 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.
2017A&A...597A..30A viz 16       D               1 607 94 Galactic archaeology with asteroseismology and spectroscopy: Red giants observed by CoRoT and APOGEE. ANDERS F., CHIAPPINI C., RODRIGUES T.S., et al.
2018AJ....156...90H viz 16       D               1 18080 37 A new catalog of radial velocity standard stars from the APOGEE data. HUANG Y., LIU X.-W., CHEN B.-Q., 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.
2019AJ....158..147H viz 17       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.
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               2 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.

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