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| TYC 3146-824-1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:37:29 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2013MNRAS.431.2240B |
15 | D | 1 | 899 | 128 | Activity in A-type stars. | BALONA L.A. | ||
|
2016A&A...594A..39F |
16 | D | 4 | 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.477.5261B | 80 | C | 1 | 57 | 8 | On the kinematics of a runaway Be star population. | BOUBERT D. and EVANS N.W. | ||
|
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. | ||
|
2019MNRAS.490.2112B |
16 | D | 1 | 2864 | ~ | Evidence for spots on hot stars suggests major revision of stellar physics. | BALONA L.A. | ||
|
2020ApJS..251...15Z |
16 | D | 1 | 20886 | 38 | Phase II of the LAMOST-Kepler/K2 survey. I. Time series of medium-resolution Spectroscopic observations. | ZONG W., FU J.-N., DE CAT P., et al. | ||
|
2020A&A...643A.122S |
16 | D | 1 | 3787 | ~ | Active deep learning method for the discovery of objects of interest in large spectroscopic surveys. | SKODA P., PODSZTAVEK O. and TVRDIK P. | ||
|
2022ApJS..259...63S |
17 | D | 1 | 10269 | 2 | Objective Separation between CP1 and CP2 Based on Feature Extraction with Machine Learning. | SHANG L.-H., LUO A.-L., WANG L., et al. | ||
|
2022A&A...664A..78F |
17 | D | 1 | 7452 | 7 | Characterization of Kepler targets based on medium-resolution LAMOST spectra analyzed with ROTFIT,. | FRASCA A., MOLENDA-ZAKOWICZ J., ALONSO-SANTIAGO J., et al. | ||
|
2023ApJS..266...14T |
17 | D | 1 | 21501 | ~ | A New Catalog of Am-type Chemically Peculiar Stars Based on LAMOST. | TIAN X.-M., WANG Z.-H., ZHU L.-Y., et al. |