TYC 3557-2030-1 , the SIMBAD biblio

TYC 3557-2030-1 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.06.13CEST01:11:44


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Title First 3 Authors
2012ApJS..199...24T viz 15       D               1 5394 66 Detection of potential transit signals in the first three quarters of Kepler mission data. TENENBAUM P., CHRISTIANSEN J.L., JENKINS J.M., et al.
2013A&A...557L..10N viz 16       D               1 12151 189 Rotation periods of 12000 main-sequence Kepler stars: dependence on stellar spectral type and comparison with v sin i observations. NIELSEN M.B., GIZON L., SCHUNKER H., et al.
2016A&A...594A..39F viz 16       D               2 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 viz 16       D               1 2598 17 Gaia luminosities of pulsating A-F stars in the Kepler field. BALONA L.A.
2019ApJ...871..193H viz 17       D               1 485 1 A combined Chandra and LAMOST study of stellar activity. HE L., WANG S., LIU J., et al.
2019MNRAS.485.2380M viz 17       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.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2020AJ....160..120J viz 17       D               1 365761 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.
2020ApJS..251...15Z viz 17       D               1 20889 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.
2022A&A...664A..78F viz 18       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.

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