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Dark creation
After the preliminary steps including addition of variance, the dark is
merely filed in the calibration system, using the frame number and the
exposure time in the name.
When multiple darks of the same exposure time form part of the same
grouped observation, these darks are averaged before filing with the
calibration system. Such averaged darks have the group number instead
of the observation number in their names.
[_AVERAGE_DARKS_ and IRCAM, UFTI, and UIST variants;
_GET_DARK_NAME_]
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ORAC-DR -- imaging data reduction
Starlink User Note 232
Malcolm J. Currie
Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
2004 June
E-mail:ussc@star.rl.ac.uk
Copyright © 2004 Particle Physics and Astronomy Research Council