Bayesian analysis of the molecular emission and dust continuum of protoplanetary disks

Home

All issues

Volume 687 (July 2024)

A&A, 687 (2024) A209

Full HTML

Open Access

Table 5

Prior parameter ranges for fitting the GW Lup’s MIRI spectrum.

Parameter	Prior	Parameter	Prior
T_rim	𝒰(10,1600)	q_emis	𝒰(−1,−0.1)
$T_{\min}^{sur}$ $T_{\min }^{{\rm{sur}}}$	𝒰(10,400)	a_obs	ℐ(10⁻⁵,10⁻¹)
$T_{\max}^{sur}$ $T_{\max }^{{\rm{sur}}}$	𝒰(300,1600)	Σ_tmin(1)	ℐ(10¹⁴,10²⁴)
$T_{min}^{mid}$ $T_{{\rm{min}}}^{{\rm{mid}}}$	𝒰(10,400)	Σ_tmax	ℐ(10¹⁴,10²⁴)
$T_{max}^{mid}$ $T_{{\rm{max}}}^{{\rm{mid}}}$	𝒰(300,1600)	T_max(1)	𝒰(25,1500)
q_mid	𝒰(−1,−0.1)	T_min(1)	𝒰(25,1500)
q_sur	𝒰(−1,−0.1)

Notes. The terms 𝒰(x, y) and 𝒯(x, y) denote uniform and log-uniform priors in the range from x to y, respectively. The units of the parameters are given in Table 2. Further linear parameters are not listed here (see text). ⁽¹⁾Same prior used for H₂O, CO₂, HCN, and C₂H₂.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.