Welcome to uvmcmcfit‘s documentation!

uvmcmcfit is Python software designed to allow users to fit parametric models to interferometric data. It is ideally suited to extract the maximum amount of information from marginally resolved observations with interferometers like the Atacama Large Millimeter Array (ALMA), Submillimeter Array (SMA), and Plateau de Bure Interferometer (PdBI).

uvmcmcfit has been thoroughly tested on continuum imaging from ALMA (Bussmann et al., in prep.), SMA (Bussmann et al. 2012, 2013), and PdBI (Miettenen et al., in prep.). It has also been tested on spectral line imaging from PdBI (Oteo et al. in prep.) and SMA (Bradli et al., in prep.).

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