Image Details
Caption: Figure 12.
Images of discovery candidate with high S/N at the beginning, middle, and end of SALTAD processing. The top row shows the raw frames as read by SALTAD with any nondata values replaced by the mean value of the subframe. The middle row shows the same images after the image equalization step. The bottom image shows the same frames after convolution with the PSF, as the frames are when they are shifted and stacked by SALTAD.
© 2026. The Author(s). Published by the American Astronomical Society.