Image Details
Caption: Figure 8.
Robustness of CKAN under JWST and Euclid noise. The network is trained on CDM-low AGN, CDM fiducial AGN, and two SIDM models (σDM/m = 0.1, 1 cm2 g−1), and then tested on the unseen CDM-hi AGN, all these with JWST and Euclid noise. A consistent sample size of n = 100 is used for all tests.
© 2025. The Author(s). Published by the American Astronomical Society.