Filter your results
- 3
- 3
- 3
- 1
- 2
- 3
- 1
- 1
- 1
- 1
- 1
- 3
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 2
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
- 1
|
|
sorted by
|
|
The Obliquity of HIP 67522 b: A 17 Myr Old Transiting Hot, Jupiter-sized PlanetThe Astrophysical Journal Letters, 2021, 922, ⟨10.3847/2041-8213/ac3485⟩
Journal articles
insu-03672381v1
|
||
|
Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type starsAstronomy and Astrophysics - A&A, 2022, 664, ⟨10.1051/0004-6361/202243454⟩
Journal articles
insu-03860318v1
|
||
|
TOI-257b (HD 19916b): a warm sub-saturn orbiting an evolved F-type starMonthly Notices of the Royal Astronomical Society, 2021, 502, pp.3704-3722. ⟨10.1093/mnras/staa3960⟩
Journal articles
insu-03713781v1
|