K2-19d , the SIMBAD biblio

K2-19d , the SIMBAD biblio (15 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST06:05:29


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Title First 3 Authors
2016ApJ...823..115D 157           X C       3 21 27 Doppler monitoring of five K2 transiting planetary systems. DAI F., WINN J.N., ALBRECHT S., et al.
2016ApJ...827...78S 134       D     X         4 49 94 Eleven multiplanet systems from K2 campaigns 1 and 2 and the masses of two hot super-earths. SINUKOFF E., HOWARD A.W., PETIGURA E.A., et al.
2016ApJS..226....7C viz 16       D               1 400 165 197 candidates and 104 validated planets in K2's first five fields. CROSSFIELD I.J.M., CIARDI D.R., PETIGURA E.A., et al.
2017A&A...601A.128N viz 79           X         2 10 10 Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations. NESPRAL D., GANDOLFI D., DEEG H.J., et al.
2018AJ....155..136M viz 16       D               1 521 127 275 candidates and 149 validated planets orbiting bright stars in K2 campaigns 0-10. MAYO A.W., VANDERBURG A., LATHAM D.W., et al.
2020AJ....159....2P viz 290           X C       6 5 12 K2-19b and c are in a 3:2 commensurability but out of resonance: a challenge to planet assembly by convergent migration. PETIGURA E.A., LIVINGSTON J., BATYGIN K., et al.
2020ApJ...897....7M 41           X         1 36 18 Tidal inflation reconciles low-density sub-Saturns with core accretion. MILLHOLLAND S., PETIGURA E. and BATYGIN K.
2020MNRAS.496.3101P 41   K                 1 7 ~ Resonance in the K2-19 system is at odds with its high reported eccentricities. PETIT A.C., PETIGURA E.A., DAVIES M.B., et al.
2022A&A...662A..15M viz 17       D               1 733 3 Tidally driven tectonic activity as a parameter in exoplanet habitability. McINTYRE S.R.N.
2022MNRAS.517.4472L 43           X         1 16 6 Apsidal alignment and anti-alignment of planets in mean-motion resonance: disc-driven migration and eccentricity driving. LAUNE J.T., RODET L. and LAI D.
2023ApJ...946...61L viz 17       D               1 257 ~ A Spectroscopic Analysis of a Sample of K2 Planet-host Stars: Stellar Parameters, Metallicities and Planetary Radii. LOAIZA-TACURI V., CUNHA K., SMITH V.V., et al.
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.
2025ApJS..278...52H 65       D     X         2 136 ~ Planet Masses, Radii, and Orbits from NASA's K2 Mission. HOWARD A.W., SINUKOFF E., BLUNT S., et al.
2025A&A...703A.167A 373           X C       7 5 ~ A decade of transit photometry for K2-19: Revised system architecture. ALMENARA J.M., MARDLING R., LELEU A., et al.
2026AJ....171...46E 250           X         5 9 ~ A Decade of Transit-timing Measurements Confirm Resonance in the K2-19 System. ENTRICAN P.M., PETIGURA E.A., PETIT A.C., et al.

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