Image Details
Caption: Figure A10.
rms deviations and their deviograms of the original (panels (a) and (b)) and interpolated (panels (c) and (d)) ALSCC ROIs. rms deviations (panel (e)) and Hurst exponents (panel (f)) are shown as a function of baseline of the original (green) and interpolated (red) ALSCC ROIs. In panel (e), the black arrow indicates that the difference between the original and interpolated ALSCC ROIs is more pronounced at shorter baselines.
© 2026. The Author(s). Published by the American Astronomical Society.