Amber offset between photo. and interf. channels
esorex amber_spectral_calibration [OPTIONS] FILE.sof
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 http://www.eso.org/sci/software/pipelines/.
Basic documentation about the EsoRex program can be found at the esorex (1) man page.
It is possible to call the pipelines from python using the python-cpl package. See http://packages.python.org/python-cpl/index.html for further information.
The other recipes of the amber pipeline are amber_calibrate(7), amber_raw_to_fitsimage(7), amber_p2vm(7), amber_BeamPos(7), amber_detector(7), amber_oimerge(7), amber_SciCal(7), amber_trf(7), amber_selector(7), amber_ascii_export(7)
Armin Gabasch <[email protected]>