VizieR Online Data Catalog: Resonant sub-Neptunes are puffier (Leleu+, 2024)
Abstract
Full sample, with robust masses from Hadden & Lithwick (2017AJ....154....5H, Cat. J/AJ/154/5) and Leleu et al. (2023A&A...669A.117L, Cat. J/A+A/669/A117) when available.
For this sample, the probability that the mass of the (nearly) resonant and non-resonant population is drawn form the same underlying population drops to pvalue=2.3e-06+2.7e-05-2.1e-06, while the rest of the explored parameters are consistent between the two sub-population. (1 data file).- Publication:
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VizieR Online Data Catalog
- Pub Date:
- July 2024
- Bibcode:
- 2024yCat..36879001L
- Keywords:
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- Stars: double and multiple;
- Exoplanets;
- Radial velocities;
- Stars: ages;
- Effective temperatures