TYC 3146-824-1 , the SIMBAD biblio

TYC 3146-824-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST20:37:29


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Bibcode/DOI Score in Title|Abstract|
Keywords
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
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Title First 3 Authors
2013MNRAS.431.2240B viz 15       D               1 899 128 Activity in A-type stars. BALONA L.A.
2016A&A...594A..39F viz 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 viz 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 viz 16       D               1 2864 ~ Evidence for spots on hot stars suggests major revision of stellar physics. BALONA L.A.
2020ApJS..251...15Z viz 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 viz 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 viz 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 viz 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 viz 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.

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