Radiative transfer model of the IM Lupi protoplanetary disc with a 3 Jupiter-mass planet, as published in Verrios et al. (2022)

Contains synthetic images of IM Lupi protoplanetary disc at wavelengths of 1.6 microns (data_1.6/RT.fits.gz), 1.25 mm (data_1250/RT.fits.gz) and a datacube of the synthetic 12CO 2-1 line emission from our model. The directory also contains the parameter files used to setup and perform the simulation (using the phantom smoothed particle hydrodynamics code: https://github.com/danieljprice/phantom) and to perform the radiative transfer, using the MCFOST code (https://github.com/cpinte/mcfost)