Bayesian model-fitting to OI-FITS-format data.
mfit is a tool for fitting simple parametrisations of the sky brightness distribution to optical (visible/IR) interferometry data. The source code is available for download, see the links below. You will need a Fortran 90/95 compiler (such as the freely-available G95) to build mfit.
Features of mfit include:
The following screen grab shows the GUI interface to mfit,
Gzipped tar file of package: mfit.tar.gz
mfit was written by Matthew Worsley, and subsequently modified by John Young. Please send bug reports and requests for new features to John Young (jsy1001 (at) cam.ac.uk).
OI Exchange Format | OLBIN