Dense Gas Toolbox v1.3
Dense Gas Toolbox
Aim
Calculate density and temperature from observed molecular emission lines,
using radiative transfer models.
Method
Our models assume that the molecular emission lines emerge from a
multi-density medium rather than from a single density alone.
The density distribution is assumed to be log-normal or log-normal with
a power-law tail.
The parameters (density, temperature and the width of density distribution)
are inferred using Bayesian statistics, i.e. Markov chain Monte Carlo (MCMC).
Results
Given an ascii table of observed molecular intensities [K km/s],
the results (mass-weighted mean density, temperature and width of the density
distribution) are saved in an output ascii file. Furthermore, diagnostic plots
are created to assess the quality of the fit/derived parameters.
THIS RELEASE
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New: The user may optionally infer the parameters (density, temperature, width of
density distribution) via application of the MCMC method. -
New: Diagnosis plots (corner plots) are produced when MCMC method is used.
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Update: Code updated to Python 3.X
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Update: Re-calculation of models, now including the following transitions:
12CO (up to J=3), 13CO (up to J=3), C18O (up to J=3), C17O (up to J=3),
HCN (up to J=3), HCO+ (up to J=3), HNC (up to J=3) and CS (up to J=3)