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: http://www.adass.org/adass/proceedings/adass94/
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Cover Illustration: Two B-band images of the Phoenix dwarf galaxy at different epochs ( top), and the difference of the two using new software to register and scale the images ( bottom left) and to match their PSFs ( bottom right). In the fully matched case about a dozen Cepheid variables are readily apparent, as is one high proper-motion star just below and left of center. Figures provided by Andrew Phillips and Lindsey Davis (see their paper ).