Continued writing on the faint-motion paper. It is funny how much there is left to do when a project is done!
Wu began working on the GALEX properties of post-starburst galaxies: They aren't detected at the MIS depth. That is good, because star-forming galaxies are detected. So a GALEX selection is likely to work, at some level. The question is, how good will it be? We would like to have a GALEX-based selection of the post-starburst galaxies so we can perform emission-line studies without worrying about the fact that the post-starbursts are selected on the basis of emission lines. Fortuitously, Christy Tremonti (Arizona) showed up at the MPIA today for a month, so she may be able to help out.
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