From the 1 of 24 papers with an AI index.
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- J. V. Loon2 profiles5 · h 22
- A. Brandeker2 profiles4 · h 34
- H. Osborn2 profiles4 · h 29
- J. V. van Loon4 · h 21
- Y. Alibert2 profiles4 · h 51
- A. Fortier2 profiles3 · h 3
- A. Hopkins2 profiles3 · h 5
- A. Leleu2 profiles3 · h 17
- D. Gandolfi3 · h 44
- F. Najarro3 · h 45
- F. Tramper3 · h 24
- G. Scandariato2 profiles3 · h 31
- Centre National de la Recherche ScientifiqueFR5 papers
- Centro de AstrobiologíaES5 papers
- Heidelberg UniversityDE5 papers
- Leiden UniversityNL5 papers
- Astronomical Institute of the Slovak Academy of SciencesSK4 papers
- Institute of AstronomyRU4 papers
- Instituto de Astrofísica de CanariasES4 papers
- Max Planck Institute for AstrophysicsDE4 papers
- National Institute for AstrophysicsIT4 papers
- Universidad de La LagunaES4 papers
- University of BernCH4 papers
- Armagh Observatory & PlanetariumGB3 papers
5 papers · 1 filter
Spin-Orbit Geometry of AU Mic b and c from Back-to-Back Transits Observed Contemporaneously with Magellan PFS, LCOGT, and CHEOPS
Zitao Lin, Gyula M. Szabó, Krzysztof Sz. ZieliÅski +37
Young planets offer a unique window into the early stages of planetary evolution. AU Mic is one of the nearest (9.8 pc) pre-main sequence stars (~20 Myr), hosting two transiting Ne…
The multi-planet system TOI-5624: Four transiting sub-Neptunes with an outer companion revealed by transit-timing variations
A. Bonfanti, D. Gandolfi, P. Leonardi +96
Following the 2022 alert of a TESS object of interest transiting TOI-5624 (a G7 V star 100 pc away), a CHEOPS campaign in 2023 detected four planetary signals at $P_b\approx3…
Long-term monitoring of WASP-19 b: Signs of apsidal precession and molecular signatures
A. R. Rajkumar, A. Bayo, P. Peng +30
With more than 6000 exoplanets discovered so far, about 12 percent are hot Jupiters. Their large sizes and short orbital periods make them valuable targets for studying planetary f…
An Adolescent and Near-Resonant Planetary System Near the End of Photoevaporation
Mu-Tian Wang, Fei Dai, Hui-Gen Liu +28
Young exoplanets provide vital insights into the early dynamical and atmospheric evolution of planetary systems. Many multi-planet systems younger than 100 Myr exhibit mean-motion…
Gas-depleted planet formation occurred in the four-planet system around the red dwarf LHS 1903
Thomas G. Wilson, Anna M. Simpson, Andrew Collier Cameron +173
Small exoplanet radii show two populations, referred to as super-Earths and sub-Neptunes, separated by a gap known as the radius valley. This may be produced by the removal of atmo…