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| TOI-920 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST18:38:19 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2018MNRAS.473.2004S |
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 |
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 |
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 |
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 |
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 |
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 |
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 |
17 | D | 1 | 114072 | 2 | Quantifying Chemical and Kinematical Properties of Galactic Disks. | HU G. and SHAO Z. | ||
|
2022MNRAS.517.5325H |
17 | D | 1 | 214414 | 23 | The GALAH survey: chemical clocks. | HAYDEN M.R., SHARMA S., BLAND-HAWTHORN J., et al. | ||
|
2023ApJ...950..142H |
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. |