TOI-920 , the SIMBAD biblio

TOI-920 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST18:38:19


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Title First 3 Authors
2018MNRAS.473.2004S viz 16       D               1 24972 89 The TESS-HERMES Survey data release 1: high-resolution spectroscopy of the TESS southern continuous viewing zone. SHARMA S., STELLO D., BUDER S., 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...901..109H viz 16       D               1 45439 31 Exploring the stellar age distribution of the Milky Way bulge using APOGEE. HASSELQUIST S., ZASOWSKI G., FEUILLET D.K., et al.
2021AJ....162..192Z viz 17       D               1 713 29 SOAR TESS survey. II. The impact of stellar companions on planetary populations. ZIEGLER C., TOKOVININ A., LATIOLAIS 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.
2022MNRAS.512L..60H viz 17       D               1 1974 9 The flaring TESS Objects of Interest: flare rates for all two-minute cadence TESS planet candidates. HOWARD W.S.
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.
2022MNRAS.517.5325H viz 17       D               1 214414 23 The GALAH survey: chemical clocks. HAYDEN M.R., SHARMA S., BLAND-HAWTHORN J., et al.
2023ApJ...950..142H viz 17       D               1 26076 ~ Angular Momentum Variation of the Milky Way Thick Disk: The Dependence of Chemical Abundance and Evidence of the Inside-out Formation Scenario. HU G., SHAO Z. and LI L.

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