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