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| CD-57 1349 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST17:31:38 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1987A&AS...71..413M |
14 | D | 1 | 31534 | 42 | UBV Photoelectric Photometry Catalogue (1986): I. The Original data. | MERMILLIOD J.C. | ||
|
2021ApJ...919..131H |
17 | D | 1 | 158508 | 22 | A "quick look" at all-sky Galactic archeology with TESS: 158,000 oscillating red giants from the MIT Quick-look Pipeline. | HON M., HUBER D., KUSZLEWICZ J.S., 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. | ||
|
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. | ||
|
2023A&A...677A..21K |
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. | ||
|
2023A&A...678A.158A |
17 | D | 1 | 171655 | ~ | Spectroscopic age estimates for APOGEE red-giant stars: Precise spatial and kinematic trends with age in the Galactic disc. | ANDERS F., GISPERT P., RATCLIFFE B., et al. | ||
| 2025ApJ...986..144M | 19 | D | 3 | 537 | ~ | Asteroseismology of Metal-poor Red Giants Observed by TESS. | MARASCO C., TAYAR J. and NIDEVER D. |