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| TYC 2666-352-1 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST18:52:13 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2004AJ....128.1761H 
|
15 | D | 1 | 1625 | 96 | HATNET variability survey in the high stellar density ``Kepler field'' with millimagnitude image subtraction photometry. | HARTMAN J.D., BAKOS G., STANEK K.Z., et al. | ||
|
2011A&A...534A.125U
|
15 | D | O | 2 | 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. | |
|
2016A&A...594A..39F
|
16 | D | 1 | 51408 | 86 | Activity indicators and stellar parameters of the Kepler targets. An application of the ROTFIT pipeline to LAMOST-Kepler stellar spectra. | FRASCA A., MOLENDA-ZAKOWICZ J., DE CAT P., et al. | ||
|
2018MNRAS.479..183B
|
16 | D | 1 | 2598 | 17 | Gaia luminosities of pulsating A-F stars in the Kepler field. | BALONA L.A. | ||
| 2019RAA....19....1Q | 97 | D | X | 3 | 172 | 1 | Physical properties of γ Doradus pulsating stars and their relationship with long-period δ Scuti variables. | QIAN S.-B., LI L.-J., HE J.-J., et al. | |
|
2019MNRAS.485.2380M
|
16 | D | 1 | 14330 | 108 | Gaia-derived luminosities of Kepler A/F stars and the pulsator fraction across the δ Scuti instability strip. | MURPHY S.J., HEY D., VAN REETH T., et al. | ||
|
2020MNRAS.491.3586L
|
16 | D | 3 | 609 | 75 | Gravity-mode period spacings and near-core rotation rates of 611 γ Doradus stars with Kepler. | LI G., VAN REETH T., BEDDING T.R., 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. | ||
|
2024A&A...684A.112F
|
18 | D | 1 | 491 | ~ | Age uncertainties of red giants due to cumulative rotational mixing of progenitors calibrated by asteroseismology. | FRITZEWSKI D.J., AERTS C., MOMBARG J.S.G., et al. |
