2022ApJ...927..203K


Query : 2022ApJ...927..203K

2022ApJ...927..203K - Astrophys. J., 927, 203-203 (2022/March-2)

UCLCHEMCMC: An MCMC Inference Tool for Physical Parameters of Molecular Clouds.

KEIL M., VITI S. and HOLDSHIP J.

Abstract (from CDS):

We present the publicly available open-source code UCLCHEMCMC, designed to estimate physical parameters of an observed cloud of gas by combining Markov chain Monte Carlo (MCMC) sampling with chemical and radiative transfer modeling. When given the observed values of different emission lines, UCLCHEMCMC runs a Bayesian parameter inference, using an MCMC algorithm to sample the likelihood and produce an estimate of the posterior probability distribution of the parameters. UCLCHEMCMC takes a full forward-modeling approach, generating model observables from the physical parameters via chemical and radiative transfer modeling. While running UCLCHEMCMC, the created chemical models and radiative transfer code results are stored in an SQL database, preventing redundant model calculations in future inferences. This means that the more UCLCHEMCMC is used, the more efficient it becomes. Using UCLCHEM and RADEX, the increase oin efficiency is nearly two orders of magnitude, going from 5185.33 ± 1041.96 s for 10 walkers to take 1000 steps when the database is empty, to 68.89 ± 45.39 s when nearly all models requested are in the database. In order to demonstrate its usefulness, we provide an example inference of UCLCHEMCMC to estimate the physical parameters of mock data, and perform two inferences on the well-studied prestellar core, L1544, one of which shows that it is important to consider the substructures of an object when determining which emission lines to use.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Astrochemistry - Interdisciplinary astronomy - Markov chain Monte Carlo - Bayesian statistics - Posterior distribution

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 LDN 1544 DNe 05 04 16.6 +25 10 48           ~ 965 0

Query : 2022ApJ...927..203K

Basic data :
LDN 1544 -- Dark Cloud (nebula)
Other object types:
otypes_help
DNe (LDN)
ICRS coord. (ep=J2000) :
05 04 16.6 +25 10 48 (Radio) [ ] D 2004ApJS..152...81P
FK4 coord. (ep=B1950 eq=1950) :
05 01 12.5 +25 06 40 [ ]
Gal coord. (ep=J2000) :
177.9797 -09.7308 [ ]
Radial velocity / Redshift / cz :
V(km/s) 6.95 [~] / z(~) 0.000023 [~] / cz 6.95 [~]
   D 1978ApJ...221L.117H
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LDN 1544

References (965 between 1850 and 2026) (Total 965)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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