This is the release repo for my synthetic CMD project that I did for my undergrad astronomy thesis. It serves as an interface between the [Astropy SPISEA package] as described in Hosek et al. 2020, and the Nbody6++ protocluster simulations as described in Farias et al. 2018, to create a diagram of the forecasted appearance of a forming star cluster.
This only contains iterations of the software and does not have any development/test code for the sake of keeping the repository clean. If you'd like to see my dev code, please see the dev repo synthetic-cmd-dev.