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| TYC 3549-2851-1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST05:01:38 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2011A&A...534A.125U 
|
15 | D | 1 | 764 | 297 | The Kepler characterization of the variability among A- and F-type stars. I. General overview. | UYTTERHOEVEN K., MOYA A., GRIGAHCENE A., et al. | ||
| 2012ApJ...751L..36W | 15 | D | 1 | 59 | 34 | Solving the mode identification problem in asteroseismology of f stars observed with Kepler. | WHITE T.R., BEDDING T.R., GRUBERBAUER M., et al. | ||
|
2016AJ....152..181H
|
16 | D | 1 | 9279 | 22 | SETI observations of exoplanets with the Allen Telescope Array. | HARP G.R., RICHARDS J., TARTER J.C., et al. | ||
|
2019ApJ...879...69T
|
16 | D | 1 | 222610 | 141 | The Payne: self-consistent ab initio fitting of stellar spectra. | TING Y.-S., CONROY C., RIX H.-W., et al. | ||
|
2020A&A...638A..59B
|
16 | D | 1 | 2220 | 17 | Unveiling the power spectra of δ Scuti stars with TESS. The temperature, gravity, and frequency scaling relation. | BARCELO FORTEZA S., MOYA A., BARRADO D., 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...930....7A
|
17 | D | 1 | 4216 | 14 | Rotation Distributions around the Kraft Break with TESS and Kepler: The Influences of Age, Metallicity, and Binarity. | AVALLONE E.A., TAYAR J.N., VAN SADERS J.L., et al. | ||
|
2023A&A...674A..34G
|
17 | D | 1 | 307215 | 85 | Gaia Data Release 3 Stellar multiplicity, a teaser for the hidden treasure. | GAIA COLLABORATION, ARENOU F., BABUSIAUX C., et al. |
