Wrote figure captions in the Barron & Stumm paper, and annotated equations in the Masjedi paper.
Jester and I discussed the problem of the determination of proper motions of sources in multi-epoch imaging, even when the sources are too faint to be detected at any single epoch. It is a beautiful statistics problem, and highly relevant to the SDSS Southern Stripe (where there are many epochs), PanSTARRS, and LSST.
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