Finally I returned to my summer project of distinguishing brown dwarfs from high-redshift quasars via proper motions. The faithful reader will recall that the method is to use proper motions determined in multi-epoch imaging in which the source of interest is not significantly detected at any single epoch. I spent the morning remembering what I had done and re-running the code on new data provided by Jester (many months ago).
No comments:
Post a Comment