58 citations
- K. Collins4 profiles69 · h 40
- C. Ziegler2 profiles64 · h 31
- J. Winn2 profiles46 · h 83
- S. Seager2 profiles45 · h 92
- J. Jenkins2 profiles43 · h 97
- G. Ricker37 · h 62
- D. Latham2 profiles33 · h 111
- S. Howell2 profiles31 · h 83
- R. Schwarz2 profiles29 · h 25
- R. Vanderspek29 · h 51
- A. Mann28 · h 51
- N. Law2 profiles26 · h 52
- Center for Astrophysics Harvard & SmithsonianUS61 papers
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- University of North Carolina at Chapel HillUS39 papers
- California Institute of TechnologyUS36 papers
- Search for Extraterrestrial IntelligenceUS35 papers
- NASA Exoplanet Science InstituteUS34 papers
- Instituto de Astrofísica de CanariasES31 papers
- Centre National de la Recherche ScientifiqueFR29 papers
- Goddard Space Flight CenterUS28 papers
76 papers
ASTEP confirmation of a pair of long-period Jupiter-sized planets with extremely low densities transiting TOI-791
Georgina Dransfield, Antoine C. Petit, Amaury H. M. J. Triaud +45
Gas giant planets with periods orbiting Sun-like stars are a relatively uncommon outcome of planetary formation, and key questions about the nature and form…
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…
The GAPS programme at TNG LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)
A. S. Bonomo, L. Naponiello, A. Sozzetti +37
Sub-Neptunes with planetary radii of are the most common planets around solar-type stars in short-period ( d) orbits. It is still unclear, howe…
A transiting hot Jupiter with two outer siblings orbiting an intermediate-mass post main-sequence star
Y. Reinarz, M. I. Jones, R. Brahm +15
Exoplanetary systems with multiple giant planets present an opportunity to understand planet formation, migration processes, and long-term system-wide dynamical interactions. In pa…
Detection and characterisation of a 106-day transiting Jupiter : TOI-2449 b / NGTS-36 b
S. Ulmer-Moll, S. Gill, R. Brahm +64
Only a handful of transiting giant exoplanets with orbital periods longer than 100 days are known. These warm exoplanets are valuable objects as their radius and mass can be measur…
Migration and Evolution of giant ExoPlanets (MEEP) II: Super-Jupiters and Lithium-rich Host Stars
Jack Schulte, Joseph E. Rodriguez, David W. Latham +30
Although hot Jupiters were the first exoplanets discovered orbiting main sequence stars, the dominant mechanisms through which they form and evolve are not known. To address the qu…