The mass-radius relation of intermediate-mass planets outlined by hydrodynamic escape and thermal evolution

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Table 2

Model boundaries for each considered T_eq interval.

	Lower boundary	Upper boundary	^Npoints
<512 K	512 K, fast rotator	-	22
512–680 K	680 K, fast rotator	512 K, slow rotator	28
680–956 K	956 K, fast rotator	680 K, slow rotator	63
956–1350 K	1350 K, fast rotator	956 K, slow rotator	54
1350–1700 K	1700 K, fast rotator	1350 K, slow rotator	16
>1700 K	–	1700 K, slow rotator	15

Notes. The last column lists the number of observed planets falling within each T_eq interval.

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