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| WASP-107c , the SIMBAD biblio (16 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST08:44:41 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2021AJ....161...70P |
169 | X | 4 | 17 | 37 | WASP-107b's density is even lower: a case study for the physics of planetary gas envelope accretion and orbital migration. | PIAULET C., BENNEKE B., RUBENZAHL R.A., et al. | ||
|
2021AJ....161..119R |
419 | X | 10 | 20 | 22 | The TESS-Keck survey. IV. A retrograde, polar orbit for the ultra-low-density, hot super-Neptune WASP-107b. | RUBENZAHL R.A., DAI F., HOWARD A.W., et al. | ||
| 2022MNRAS.513.5290D | 17 | D | 2 | 97 | 2 | A target list for searching for habitable exomoons. | DOBOS V., HARIS A., KAMP I.E.E., et al. | ||
| 2023A&A...669A..63B | 218 | X | 5 | 44 | 5 | DREAM I. Orbital architecture orrery. | BOURRIER V., ATTIA O., MALLONN M., et al. | ||
| 2023MNRAS.521.3663B | 44 | X | 1 | 38 | 8 | The occurrence rate of giant planets orbiting low-mass stars with TESS. | BRYANT E.M., BAYLISS D. and VAN EYLEN V. | ||
| 2023ApJ...949...79H | 174 | S X | 3 | 3 | ~ | Elemental Abundances of the Super-Neptune WASP-107b's Host Star Using High-resolution, Near-infrared Spectroscopy. | HEJAZI N., CROSSFIELD I.J.M., NORDLANDER T., et al. | ||
| 2024Natur.630..831S | 45 | X | 1 | 7 | ~ | A warm Neptune's methane reveals core mass and vigorous atmospheric mixing. | SING D.K., RUSTAMKULOV Z., THORNGREN D.P., et al. | ||
| 2024ApJ...972..159Y | 251 | A | S X | 5 | 9 | ~ | Are WASP-107-like Systems Consistent with High-eccentricity Migration? | YU H. and DAI F. | |
| 2024NatAs...8.1562M | 45 | X | 1 | 7 | ~ | Evidence for morning-to-evening limb asymmetry on the cool low-density exoplanet WASP-107 b. | MURPHY M.M., BEATTY T.G., SCHLAWIN E., et al. | ||
|
2025A&A...693A.285S |
19 | D | 1 | 221 | ~ | Connection between planetary He I λ10 830 Å absorption and extreme-ultraviolet emission of planet-host stars. | SANZ-FORCADA J., LOPEZ-PUERTAS M., LAMPON M., et al. | ||
| 2025ApJ...985...87B | 75 | A | X | 2 | 6 | ~ | From Tides to Currents: Unraveling the Mechanism that Powers WASP-107b's Internal Heat Flux. | BATYGIN K. | |
| 2025ApJS..278...52H | 47 | X | 1 | 136 | ~ | Planet Masses, Radii, and Orbits from NASA's K2 Mission. | HOWARD A.W., SINUKOFF E., BLUNT S., et al. | ||
| 2025ApJ...986..117Y | 93 | X | 2 | 18 | ~ | A Third Star in the HAT-P-7 System and a New Dynamical Pathway to Misaligned Hot Jupiters. | YANG E., SU Y. and WINN J.N. | ||
| 2025ApJ...988..247S | 47 | X | 1 | 31 | ~ | Tidal Inflation is Stronger for Misaligned Neptune-sized Planets Than Aligned Ones. | SETHI R. and MILLHOLLAND S.C. | ||
| 2026ApJ...996L..28W | 200 | X | 4 | 6 | ~ | Evidence for a Nonzero Eccentricity Superpuff Exoplanet WASP-107 b Using JWST Occultation Observation. | WU Y., ZHANG Z., MA X., et al. | ||
| 2026ApJ..1000L..54Y | 300 | X C | 5 | 7 | ~ | “Popcorn Planets” Are Not Actively Inflated by Eccentricity Tides. | YEE S.W. and VISSAPRAGADA S. |