Image Details
Caption: Figure 7.
Flux agreement between ramp-fit and group-difference estimates for our candidate moving sources (see Tables 3 and 4). Only sources with SNR > 5 in both the ramp-fit and group-differenced images are plotted here. All magnitudes agree within their uncertainties, demonstrating that flux is conserved across both image calibrations.
© 2026. The Author(s). Published by the American Astronomical Society.