Image Details
Caption: Figure 8.
The likelihood function ﹩P({\widehat{D}}_{T}| {{\rm{\Delta }}}_{x},{{\rm{\Delta }}}_{y},{\alpha }_{r},{\alpha }_{n})﹩, similar to Figure 7 but evaluated for simulation 8, where the translation length is smaller than the resolving width of the PSFs.
© 2024. The Author(s). Published by the American Astronomical Society.