K2-138e , the SIMBAD biblio

K2-138e , the SIMBAD biblio (22 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST10:29:38

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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
2018AJ....155...57C 81             C       1 34 51 The K2-138 system: a near-resonant chain of five sub-Neptune planets discovered by citizen scientists. CHRISTIANSEN J.L., CROSSFIELD I.J.M., BARENTSEN G., et al.
2019A&A...631A..90L viz 83             C       1 10 24 Exoplanet characterisation in the longest known resonant chain: the K2-138 system seen by HARPS. LOPEZ T.A., BARROS S.C.C., SANTERNE A., et al.
2020AJ....159..207B 16       D               1 150 ~ Transit duration variations in multiplanet systems. BOLEY A.C., VAN LAERHOVEN C. and GRANADOS CONTRERAS A.P.
2020AJ....159..239G viz 16       D               1 1408 ~ Updated parameters and a new transmission spectrum of HD 97658b. GUO X., CROSSFIELD I.J.M., DRAGOMIR D., et al.
2020A&A...642A.173N 83           X         2 35 53 The CARMENES search for exoplanets around M dwarfs. Two planets on opposite sides of the radius gap transiting the nearby M dwarf LTT 3780. NOWAK G., LUQUE R., PARVIAINEN H., et al.
2021AJ....161..219H 184       D     X C       4 21 6 K2-138 g: Spitzer spots a sixth planet for the citizen science system. HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., CIARDI D.R., et al.
2021A&A...652A.110L 17       D               1 82 7 Why do more massive stars host larger planets? LOZOVSKY M., HELLED R., PASCUCCI I., et al.
2021ApJ...921...24S viz 17       D               1 328 1 The occurrence-weighted median planets discovered by transit surveys orbiting solar-type stars and their implications for planet formation and evolution. SCHLAUFMAN K.C. and HALPERN N.D.
2022A&A...657A.102M viz 298     A D S   X         7 11 ~ Detection capability of ground-based meter-sized telescopes for shallow exoplanet transits. MALLONN M., POPPENHAEGER K., GRANZER T., et al.
2022AJ....163..162M 954       D     X C       22 11 4 Confirming the 3:2 Resonance Chain of K2-138. MacDONALD M.G., FEIL L., QUINN T., et al.
2022A&A...660A.102A viz 17       D               1 37 4 Water content trends in K2-138 and other low-mass multi-planetary systems. ACUNA L., LOPEZ T.A., MOREL T., et al.
2023ApJ...954...57C 17       D               1 14 ~ A Six-planet Resonance Chain in K2-138? CERIONI M. and BEAUGE C.
2023A&A...677A.160C 1262     A D S   X C F     27 40 ~ Tidal interactions shape period ratios in planetary systems with three-body resonant chains. CHARALAMBOUS C., TEYSSANDIER J. and LIBERT A.-S.
2024ApJ...961..203M 108       D         F     2 50 ~ Spin Dynamics of Planets in Resonant Chains. MILLHOLLAND S.C., LARA T. and TOOMLAID J.
2024ApJ...966..185C 18       D               1 140 ~ Where Are the Water Worlds? Identifying Exo-water-worlds Using Models of Planet Formation and Atmospheric Evolution. CHAKRABARTY A. and MULDERS G.D.
2024A&A...685A.143M viz 18       D               1 535 ~ Planets similar in size are often dissimilar in interior. MAMONOVA E., SHAN Y., HATALOVA P., et al.
2024MNRAS.531.3698H 206 ~ Shallower radius valley around low-mass hosts: evidence for icy planets, collisions, or high-energy radiation scatter. HO C.S.K., ROGERS J.G., VAN EYLEN V., et al.
2024A&A...687L...1L viz 18       D               2 140 ~ Resonant sub-Neptunes are puffier. LELEU A., DELISLE J.-B., BURN R., et al.
2024A&A...688A.192V 90               F     3 15 ~ New ephemerides and detection of transit-timing variations in the K2-138 system using high-precision CHEOPS photometry. VIVIEN H.G., HOYER S., DELEUIL M., et al.
2025ApJ...987...85R 19       D               1 241 ~ Characterizing Exoplanets for Assessing Their Potential Habitability. RODRIGUEZ-MOZOS J.M. and MOYA A.
2025ApJS..281...61L 19       D               1 643 ~ Stellar Characterization, Magnesium Abundances, and Chromospheric Activity Analysis of Stars with Confirmed Exoplanets from the K2 Mission. LOAIZA-TACURI V., SOUTO D., QUISPE-HUAYNASI F., et al.
2026ApJ...996...12K 50           X         1 19 ~ Higher-order Mean-motion Resonances Can Form in Type I Disk Migration. KELLER F.M., DAI F. and XU W.

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