2MASS J18544461+4820247 , the SIMBAD biblio

2MASS J18544461+4820247 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST14:44:46

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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
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.
2014AJ....147...45C viz 15       D               1 1280 133 Kepler eclipsing binary stars. IV. Precise eclipse times for close binaries and identification of candidate three-body systems. CONROY K.E., PRSA A., STASSUN K.G., et al.
2014MNRAS.437.3473A viz 15       D               1 2614 45 A catalogue of temperatures for Kepler eclipsing binary stars. ARMSTRONG D.J., GOMEZ MAQUEO CHEW Y., FAEDI F., et al.
2014AJ....147..119C viz 15       D               1 8013 91 Contamination in the Kepler field. Identification of 685 KOIs as false positives via ephemeris matching based on Q1-Q12 data. COUGHLIN J.L., THOMPSON S.E., BRYSON S.T., et al.
2016AJ....151...68K viz 16       D               1 2915 316 Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data set. KIRK B., CONROY K., PRSA A., et al.
2016ApJS..224...12C viz 16       D               1 1111 211 Planetary candidates observed by Kepler VII. The first fully uniform catalog based on the entire 48-month data set (Q1-Q17 DR24). COUGHLIN J.L., MULLALLY F., THOMPSON S.E., et al.
2016ApJ...824...15V viz 16       D               1 982 20 Orbital circularization of hot and cool Kepler eclipsing binaries. VAN EYLEN V., WINN J.N. and ALBRECHT S.
2016A&A...594A..39F viz 16       D               3 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.
2016AJ....152..158T viz 16       D               1 4388 37 Detection of potential transit signals in 17 quarters of Kepler data: results of the final Kepler mission transiting planet search (DR25). TWICKEN J.D., JENKINS J.M., SEADER S.E., et al.
2017MNRAS.467.1830B viz 16       D               1 642 26 Starspots on A stars. BALONA L.A.
2018A&A...619A..98H 16       D               4 70 27 The Kepler view of magnetic chemically peculiar stars. HUMMERICH S., MIKULASEK Z., PAUNZEN E., et al.
2019ApJS..244...43Z viz 16       D               1 1328 22 Unbiased distribution of binary parameters from LAMOST and Kepler observations. ZHANG J., QIAN S.-B., WU Y., et al.
2020A&A...640A..40H viz 16       D               1 1016 21 A plethora of new, magnetic chemically peculiar stars from LAMOST DR4. HUMMERICH S., PAUNZEN E. and BERNHARD K.
2021A&A...652A.120I viz 17       D               1 3434 18 An all-sky sample of intermediate- to high-mass OBA-type eclipsing binaries observed by TESS. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.
2022ApJS..259...63S viz 17       D               3 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.
2022ApJS..262...10K viz 43           X         1 278 6 Characteristics of Kepler Eclipsing Binaries Displaying a Significant O'Connell Effect. KNOTE M.F., CABALLERO-NIEVES S.M., GOKHALE V., et al.
2023ApJ...943..147S viz 44           X         1 22 ~ An Ap Star Catalog Based on LAMOST DR9. SHI F., ZHANG H., FU J., et al.
2023A&A...676A..55L viz 17       D               1 790 ~ Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS. LABADIE-BARTZ J., HUMMERICH S., BERNHARD K., et al.
2024A&A...685A..62I viz 18       D               1 2906 ~ Automated eccentricity measurement from raw eclipsing binary light curves with intrinsic variability. IJSPEERT L.W., TKACHENKO A., JOHNSTON C., et al.
2025MNRAS.538.3247B 299       D     X   F     6 37 ~ GALEX UV survey of magnetic chemically peculiar stars in the Kepler prime field. BERTONE E., HUMMERICH S., CHAVEZ M., et al.

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