Modelling the Milky Way’s exoplanet population based on cosmological galaxy simulations

Open Access

Table A.1

Parameters of the bivariate Gaussian distributions in the mass-period diagram.

planet type	μ_P [days]	μ_M [M_⊕]	σ_P	σ_M	ρ
hot Jupiters (HJ)	log(4 ∙ 10⁰)	log(2 ∙ 10²)	0.2	0.4	−0.6
cold Jupiters (CJ)	log(5 ∙ 10²)	log(7 ∙ 10²)	0.6	0.6	0
SE & Neptunes	log(1 ∙ 10¹)	log(1 ∙ 10¹)	0.5	0.3	0.4
Earth-like	log(1 ∙ 10²)	log(1 ∙ 10⁰)	0.8	0.3	0

Notes. μ_P and μ_M are the means of the period and mass distribution, respectively in days and in Earth mass. σ_P and σ_M are the respective dispersions, and ρ is a correlation value.

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