light deconvolution

The post-Lucky imaging pipeline that Foreman-Mackey and I are writing can be thought of as light deconvolution because it builds a deconvolved model of everything, but not all the way to infinite resolution. Today, the two of us spoke with Marshall and Cato Sandford (NYU) about doing the same on PanSTARRS and CS82 data to make constant-PSF human-viewable visualizations of single and multi-epoch multi-filter data sets. This might be Stanford's first project for this summer. We also worked on code and plotting improvements for our post-Lucky software, or really on the design thereof.