A sub-Saturn mass-radius desert for planets with equilibrium temperature <600 K

Author:

Russell David G.

Funder

National Aeronautics and Space Administration

California Institute of Technology

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference44 articles.

1. The NASA exoplanet archive: data and tools for exoplanet research;Akeson;Publ. Astron. Soc. Pac.,2013

2. TOI-3884 b: a rare 6-R⊕ planet that transits a low-mass star with a giant and likely polar spot;Almenara;Astron. Astrophys.,2022

3. A remnant planetary core in the hot-Neptune desert;Armstrong;Nature,2020

4. A numerical inversion of m sin i exoplanet distribution: the sub-Saturn desert is more depleted than observed and hint of a Uranus mass gap;Bertaux;Mon. Not. R. Astron. Soc.,2022

5. Cold Jupiters and Improved Masses in 38 Kepler and K2 Small-Planet Systems From 3661 High-Precision HARPS-N Radial Velocities. No Excess of Cold Jupiters in Small-Planet Systems;Bonomo,2023

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