Revisiting the conundrum of the sub-Jovian and Neptune desert - A new approach that incorporates stellar properties

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Table 1

Samples defined in this work and their description.

Name	# planets	Description	Notes
S₁	1527	Planets with ∆R_p /R_p, ∆P/P, ∆M_* /M_, ∆R_ /R_* and ∆T_* /T_* < 10%	Sect. 2
S₂(⊂S₁)	609	S₁ planets with known mass (∆M_p /M_p < 30%	Sect. 2.3
S₃(⊂S₂)	512	S₂ planets with Mp < 600 M_⊕	Sect. 2.3

Notes. The column notes indicate where the corresponding sample is defined.

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