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Orient Image Normally
Some instruments are set up such that the spectrum on the detector
runs from higher wavelength to lower wavelength as pixel value in
increased, which is reverse to expectations. This step flips
the image so that the shorter wavelength is to the left and longer
is to the right.
[_ORIENT_IMAGE_NORMALLY_]
Next: Wavelength Calibrate
Up: Preparation of Single Frames
Previous: Interleave and Coadd
ORAC-DR -- spectroscopy data reduction
Starlink User Note 236
Paul Hirst
Brad Cavanagh
Joint Astronomy Centre, Hilo, Hawaii
October 2005
E-mail:ussc@star.rl.ac.uk
Copyright © 2005 Particle Physics and Astronomy Research Council