Description:
This primitive makes a master dark from the current group. The primitive files the
resultant dark in its calibration index.
Notes:
-
This primitive is suitable for optical imaging instruments.
-
Processing only occurs for dark frames, and when the steering header MAKE_DARK is
true.
-
The dark is displayed.
Output Data
The masterdark. It is called
"dark_instrument_UT
night_binXbinxYbin"
where instrument
is the LCOGT instrument identifier and
Xbin,
Ybin
are the binning factors in X and Y.
Tasks
CCDPACK: MAKEDARK; KAPPA: FITSMOD, NDFCOPY.
Copyright © 2014–2015 Las Cumbres Observatory Global Telescope Inc.