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| 2MASS J13443497-1657325 , the SIMBAD biblio (8 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST07:24:57 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
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. | ||
|
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. | ||
| 2022MNRAS.514.2527B | 102 | D | X | 3 | 73 | 12 | Age determination of galaxy merger remnant stars using asteroseismology. | BORRE C.C., AGUIRRE BORSEN-KOCH V., HELMI A., et al. | |
|
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. | ||
|
2024AJ....167...50S
|
18 | D | 1 | 7678 | ~ | The APO-K2 Catalog. I. ∼7500 Red Giants with Fundamental Stellar Parameters from APOGEE DR17 Spectroscopy and K2-GAP Asteroseismology. | SCHONHUT-STASIK J., ZINN J.C., STASSUN K.G., et al. | ||
|
2024A&A...683L..11V
|
18 | D | 1 | 1441 | ~ | Gaia's brightest very metal-poor (VMP) stars Metallicity catalogue of a thousand VMP stars from Gaia's radial velocity spectrometer spectra. | VISWANATHAN A., STARKENBURG E., MATSUNO T., et al. | ||
|
2024AJ....167..208W
|
18 | D | 1 | 8370 | ~ | The APO-K2 Catalog. II. Accurate Stellar Ages for Red Giant Branch Stars across the Milky Way. | WARFIELD J.T., ZINN J.C., SCHONHUT-STASIK J., et al. |
