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| UCAC4 326-081509 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST19:17:56 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2016AJ....152...75O 
|
16 | D | 1 | 358 | 2 | A wide-field survey for transiting Hot Jupiters and eclipsing pre-main-sequence binaries in young stellar associations. | OELKERS R.J., MACRI L.M., MARSHALL J.L., et al. | ||
|
2018AJ....156...76L
|
16 | D | 1 | 3079 | 34 | New young stars and brown dwarfs in the Upper Scorpius association. | LUHMAN K.L., HERRMANN K.A., MAMAJEK E.E., et al. | ||
|
2020AJ....160..120J
|
16 | D | 2 | 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. | ||
|
2021MNRAS.506..150B
|
17 | D | 1 | 588596 | 276 | The GALAH+ survey: Third data release. | BUDER S., SHARMA S., KOS J., 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. | ||
|
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. |
