Modeling the molecular gas content and CO-to-H2 conversion factors in low-metallicity star-forming dwarf galaxies

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Table 3

Distribution of parameters adopted in the broken power-law configuration.

Parameters	Statistical distribution⁽¹⁾
n	; [n_min, n_max]

U	; [U_min, U_max]

Cut	; [cut_min, cut_IF]
	; [cut_IF, cut_max]

Random variables	Priors ⁽²⁾

α_n	𝒩(µ= −1.5, σ=2)
log n_min	𝒩(µ=0, σ=1)
log n_max	𝒩(µ=4, σ=1)
α_U	𝒩(µ= −1.5, σ=2)
log U_min	𝒩(µ= −4 σ=1)
log U_max	𝒩(µ=0, σ=1)
α_cut,1	𝒩(µ=0, σ=2)
α_cut,2	𝒩(µ=0, σ=2)
cut_min	𝒩(µ=0, σ=1)
cut_max	𝒩(µ=2, σ=1)

Notes. ⁽¹⁾ ϕ_X is the statistical distribution assumed for parameter X. ⁽²⁾ 𝒩(µ, σ) is a Normal distribution with mean µ and full-width half maximum σ.

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