K2-19c , the SIMBAD biblio

K2-19c , the SIMBAD biblio (30 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:41:54


Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
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 viz 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 viz 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 viz 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 viz 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 viz 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 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.
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 viz 17       D               1 371 71 An updated study of potential targets for Ariel. EDWARDS B., MUGNAI L., TINETTI G., et al.
2019ApJS..244...11K viz 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 viz 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 viz 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 viz 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 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.
2021AJ....162..259Z viz 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.

goto View the references in ADS