HDF data were reduced with the same software as the standard HST pipeline
(the STSDAS task calwp2), but with different calibration files, and
with a slightly different treatment of the darktime. After pipeline
processing, the data were stacked and cosmic rays were identified.
Hot pixels were identified from dark frames and from the images themselves.
Details are listed below.
Copyright © 1997 The Association of Universities for
Research in Astronomy, Inc. All Rights Reserved.
There is room for improvement in all these procedures. A number
of shortcuts were taken
in the initial processing of the data.
Our plans for reprocessing the data are
evolving daily, and we would appreciate any comments.
Harry Ferguson ferguson@stsci.edu
1/14/96