The Photometric Survey
5 broad-band filters ( u', g', r', i', z’ )
limiting magnitudes (22.3, 23.3, 23.1, 22.3, 20.8)
drift scan of 10,000 square degrees
40 TB raw imaging data -> pipeline ->
calibration to 2% at r'=19.8
only done in the best seeing (20 nights/yr)
pixel size is 0.4 arcsec, astrometric precision is 60 milliarcsec
multiple scans (> 30 times) of the same stripe
Continuous data rate of 8 Mbytes/sec