Significant improvements to postprocessing scripts, which allow the user to recalculate the radiative fluxes from a PROTEUS using a high resolution spectral file. This can now be applied to a grid of models more easily, with the grid points run in parallel.
Added common telescope bandpasses to plot.py for easy comparison between model results and telescope instruments
Model calculates the bulk density that would be observed in transmission, at runtime. Stored in the helpfile alongside other variables.
Safety checks for when hydrostatic integration fails with JANUS. Does not attempt to calculate observables in these cases, since they are meaningless.
Downloads surface albedo data from OSF (closes #178). Full functionality on this part depends on #74.
plot.pyfor easy comparison between model results and telescope instruments