KOI-5106 , the SIMBAD biblio

KOI-5106 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.23CEST19:19:46


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Title First 3 Authors
2014AJ....148...38M viz 16       D               1 2648 65 WIYN open cluster study. LX. Spectroscopic binary orbits in NGC 6819. MILLIMAN K.E., MATHIEU R.D., GELLER A.M., et al.
2015AJ....149..121L viz 16       D               1 338 16 Spectroscopic abundances in the open cluster NGC 6819. LEE-BROWN D.B., ANTHONY-TWAROG B.J., DELIYANNIS C.P., et al.
2015ApJS..217...31M viz 16       D               1 2033 213 Planetary candidates observed by Kepler. VI. Planet sample from Q1–Q16 (47 months). MULLALLY F., COUGHLIN J.L., THOMPSON S.E., et al.
2015ApJ...807..170H viz 16       D               1 2117 10 Time variation of Kepler transits induced by stellar Spots–A way to distinguish between prograde and retrograde motion. II. Application to KOIs. HOLCZER T., SHPORER A., MAZEH T., et al.
2015ApJ...809....8B viz 16       D               1 112329 282 Terrestrial planet occurrence rates for the Kepler GK dwarf sample. BURKE C.J., CHRISTIANSEN J.L., MULLALLY F., et al.
2015RAA....15.2193G viz 16       D               1 539 3 3D cluster members and near-infrared distance of open cluster NGC 6819. GAO X.-H., XU S.-K. and CHEN L.
2016ApJS..225....9H viz 16       D               2 2132 124 Transit timing observations from Kepler. IX. Catalog of the full long-cadence data set. HOLCZER T., MAZEH T., NACHMANI G., et al.
2017MNRAS.465.2634A viz 16       D               1 5400 21 Transit shapes and self-organizing maps as a tool for ranking planetary candidates: application to Kepler and K2. ARMSTRONG D.J., POLLACCO D. and SANTERNE A.
2019AJ....158..163D viz 17       D               1 357 ~ Li evolution and the open cluster NGC 6819: a correlation between Li depletion and spindown in dwarfs more massive than the F-dwarf Li-dip. DELIYANNIS C.P., ANTHONY-TWAROG B.J., LEE-BROWN D.B., et al.
2021AJ....162...98B viz 17       D               1 2175 ~ Seeking echoes of circumstellar disks in Kepler light curves. BROMLEY B.C., LEONARD A., QUINTANILLA A., et al.

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