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K2-19c , the SIMBAD biblio (30 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:41:54 |
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 |
---|---|---|---|---|---|---|---|---|---|
2015ApJ...806..215F | 16 | D | 1 | 67 | 104 | A systematic search for transiting planets in the K2 data. | FOREMAN-MACKEY D., MONTET B.T., HOGG D.W., et al. | ||
2015ApJ...811..102P | 42 | X | 1 | 11 | 49 | Two transiting earth-size planets near resonance orbiting a nearby cool star. | PETIGURA E.A., SCHLIEDER J.E., CROSSFIELD I.J.M., et al. | ||
2015A&A...582A..33A | 383 | T A | X C | 8 | 7 | 30 |
One of the closest exoplanet pairs to the 3:2 mean motion resonance: K2-19b and c. |
ARMSTRONG D.J., SANTERNE A., VERAS D., et al. | |
2015MNRAS.454.4267B | 422 | A | X C | 10 | 11 | 27 | Photodynamical mass determination of the multiplanetary system K2-19. | BARROS S.C.C., ALMENARA J.M., DEMANGEON O., et al. | |
2015ApJ...815...47N | 1136 | K A | S X C | 27 | 19 | 15 | Characterization of the K2-19 multiple-transiting planetary system via high-dispersion spectroscopy, AO imaging, and transit timing variations. | NARITA N., HIRANO T., FUKUI A., et al. | |
2016ApJ...823..115D | 282 | X | 7 | 21 | 27 | Doppler monitoring of five K2 transiting planetary systems. | DAI F., WINN J.N., ALBRECHT S., et al. | ||
2016ApJ...825...76W | 6 | ~ | Detecting planet pairs in mean motion resonances via the astrometry method. | WU D.-H., LIU H.-G., YU Z.-Y., et al. | |||||
2016ApJ...827...78S | 178 | D | X | 5 | 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 | 56 | D | X | 2 | 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. | |
2016ApJ...831...64T | 20 | D | 1 | 49 | 237 | The mass-metallicity relation for giant planets. | THORNGREN D.P., FORTNEY J.J., MURRAY-CLAY R.A., et al. | ||
2017ApJ...834...17C | 17 | D | 1 | 290 | 454 | Probabilistic forecasting of the masses and radii of other worlds. | CHEN J. and KIPPING D. | ||
2017ApJ...839L...8M | 18 | D | 1 | 14 | 31 | The planetary mass-radius relation and its dependence on orbital period as measured by transit timing variations and radial velocities. | MILLS S.M. and MAZEH T. | ||
2017PASJ...69...29N | 42 | X | 1 | 5 | 5 | The K2-ESPRINT project. VI. K2-105 b, a hot Neptune around a metal-rich G-dwarf. | NARITA N., HIRANO T., FUKUI A., et al. | ||
2017AJ....153..224M | 44 | X | 1 | 11 | 37 | The Kepler-19 system: a thick-envelope super-Earth with two Neptune-mass companions characterized using radial velocities and transit timing variations. | MALAVOLTA L., BORSATO L., GRANATA V., et al. | ||
2017A&A...601A.128N | 1528 | T A | X C | 36 | 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. | ||
2019MNRAS.484.3233B | 84 | F | 1 | 35 | 5 | HARPS-N radial velocities confirm the low densities of the Kepler-9 planets. | BORSATO L., MALAVOLTA L., PIOTTO G., et al. | ||
2019AJ....157..242E | 17 | D | 1 | 371 | 71 | An updated study of potential targets for Ariel. | EDWARDS B., MUGNAI L., TINETTI G., et al. | ||
2019ApJS..244...11K | 17 | D | 1 | 2120 | 48 | Detection of hundreds of new planet candidates and eclipsing binaries in K2 campaigns 0-8. | KRUSE E., AGOL E., LUGER R., et al. | ||
2019A&A...630A.135U | 17 | D | 1 | 501 | 16 | Beyond the exoplanet mass-radius relation. | ULMER-MOLL S., SANTOS N.C., FIGUEIRA P., et al. | ||
2019MNRAS.489.3149S | 59 | D | X | 2 | 66 | ~ | Estimation of singly transiting K2 planet periods with Gaia parallaxes. | SANDFORD E., ESPINOZA N., BRAHM R., et al. | |
2020AJ....159....2P | 2471 | T A | D | X C | 57 | 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. |
2020AJ....159..120L | 43 | X | 1 | 18 | ~ | It takes two planets in resonance to tango around K2-146. | LAM K.W.F., KORTH J., MASUDA K., et al. | ||
2020ApJ...897....7M | 485 | D | X C | 11 | 36 | 18 | Tidal inflation reconciles low-density sub-Saturns with core accretion. | MILLHOLLAND S., PETIGURA E. and BATYGIN K. | |
2020MNRAS.496.3101P | 43 | 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. | ||
2021ApJ...921...24S | 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. | ||
2021AJ....162..259Z | 17 | D | 1 | 1094 | 12 | Scaling K2. IV. A uniform planet sample for Campaigns 1-8 and 10-18. | ZINK J.K., HARDEGREE-ULLMAN K.K., CHRISTIANSEN J.L., et al. | ||
2022ApJ...924....9H | 45 | X | 1 | 17 | 10 | Sculpting the sub-Saturn occurrence rate via atmospheric mass loss. | HALLATT T. and LEE E.J. | ||
2022MNRAS.517.4472L | 179 | X | 4 | 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. | ||
2023A&A...676L...8V | 19 | D | 1 | 10 | ~ | Rocky sub-Neptunes formed by pebble accretion: Rain of rock from polluted envelopes. | VAZAN A. and ORMEL C.W. |