amber_spectral_calibration - AMBER Offset between photo. and interf. channels
The recipe calculates the real Y offset between the different photometric and
the interferometric channels in the 3-telescope mode. It uses the same
algorithm as the amber_p2vm recipe.
DO category: Type: Explanation: Required:
AMBER_BADPIX Products Bad pixel map Y
AMBER_FLATFIELD Products Flatfield Y
AMBER_3WAVE Raw amber_wave data Y
DO category: Data type: Explanation:
AMBER_SPECTRAL_CALIBRATION Products Header with QC parameter
Note that it is possible to create a configuration file containing these
options, along with suitable default values. Please refer to the details
provided by the 'esorex --help' command.
The full documentation for the amber pipeline can be downloaded as a PDF file
using the following URL:
An overview over the existing ESO pipelines can be found on the web page
Basic documentation about the EsoRex program can be found at the esorex (1) man
It is possible to call the pipelines from python using the python-cpl package.
The other recipes of the amber pipeline are amber_BeamPos
Armin Gabasch <firstname.lastname@example.org>
Please report any problems to email@example.com. Alternatively, you may send a
report to the ESO User Support Department <firstname.lastname@example.org>.