Image Details
Caption: Figure 9.
Hyperparameter tuning of the regularization parameter α across varying numbers of components, n, for the sparse PCA algorithm. Reconstructions shown correspond to a selected channel from the G34.30 (top) and LkCa 15 (bottom) datasets. Nonconvergent results are labeled “DNC” (did not converge).
© 2026. The Author(s). Published by the American Astronomical Society.