Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models

Data required to recreate the plots from the paper Newman et al. 2025, "Cloudy-Maraston: Integrating nebular continuum and line emission with the Maraston stellar population synthesis models". These are grids of stellar population models that have been run through the photoionization code Cloudy . For more details, please see the paper. Additionally, a set of Jupyter notebooks have also been created to enable others to easily reproduce the plots in this paper using the provided data. These can be found at https://github.com/sophie-newman/cloudy-maraston .