Version of AGNSED (see Kubota & Done 2018) adapted to use with AGN microlensing studies. For a given SED model contains methods for: extracting 2D emissivity maps, convolving with a source-plane magnification map, estimating single-epoch magnificaiton by placing the source at some location in a magnificaiton map, and estimating microlensing variability by propagating the source across a mangification map.
This code also contains a wrapper that calls CLOUDY (Ferland et al. 2017), and handles the output, such that for a given intrinsic SED model one can estimate the contribution from the diffuse continuum. This can also be propagated through to the microlensing predictions.
Detailed documentaion coming soon. For now, see the example scripts located in the examples directory
For details, or if you use the code, please see/cite Hagen & Fian 2026 (submitted)