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[ascl:2006.003] KinMS: Three-dimensional kinematic modeling of arbitrary gas distributions

The KinMS (KINematic Molecular Simulation) package simulates observations of arbitrary molecular/atomic cold gas distributions from interferometers and line observations from integral field units. This modeling tool is optimized for situations where one has analytic forms for e.g. the rotation curve and/or surface brightness profiles (and may want to fit the parameters of these parametric models). It can, however, also be used as a tilted-ring modelling code. The routines are flexible and have been used in various different applications, including investigating the kinematics of molecular gas in early-type galaxies and determining supermassive black-hole masses from CO interferometric observations. They are also useful for creating mock observations from hydrodynamic simulations, and input data-cubes for further simulation in, for example, CASA's (ascl:1107.013) sim_observe tool. Interactive Data Language (IDL) and Python versions of the code are available.

Code site:
https://github.com/TimothyADavis/KinMSpy https://github.com/TimothyADavis/KinMS http://www.astro.cardiff.ac.uk/pub/Tim.Davis/code.php
Used in:
https://ui.adsabs.harvard.edu/abs/2013MNRAS.429..534D https://ui.adsabs.harvard.edu/abs/2017MNRAS.468.4675D
Bibcode:
2020ascl.soft06003D

Views: 361

ascl:2006.003
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