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The intensity of the background night sky now needs to be estimated and
subtracted from each of the aligned arrays. The sky may be polarized, and
so this needs to be performed independently within each of the aligned arrays.
Next: Estimation of the Stokes Parameters
Up: The Data Reduction
Previous: Image Alignment
POLPACK
Starlink User Note 223
D.S. Berry & T.M. Gledhill
26th February 2003
E-mail:ussc@star.rl.ac.uk
Copyright © 2008 Science and Technology Facilities Council