Image Details
Caption: Figure B3.
Results of the MCMC-GALFIT analysis used to constrain the photometric uncertainties of the best-fit point-source magnitudes for all three filters of UGC3478 (left: F225W; middle: F435W; right: F814W). This shows the point-source magnitudes from 500 realizations.
© 2026. The Author(s). Published by the American Astronomical Society.