Image Details
Caption: Figure 2.
Workflow of the method proposed in this paper, featuring the CNN at the center. Above the dashed line, the generation of the parameters with ronswanson, the computation of the spectra with SOPRANO, and the training of the CNN are depicted. Below the dashed line, the figure shows the CNN central to the fitting procedure, with MultiNest used for sampling the posterior distributions.
© 2024. The Author(s). Published by the American Astronomical Society.