amber_spectral_calibration (7)

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.

Input files:

  DO category:               Type:      Explanation:      Required:
  AMBER_BADPIX               Products   Bad pixel map              Y
  AMBER_FLATFIELD            Products   Flatfield                  Y
  AMBER_3WAVE                Raw        amber_wave data            Y

Output files:

  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:

• ftp://ftp.eso.org/pub/dfs/pipelines/amber/amber-pipeline-manual-4.3.1.pdf

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)

amber_spectral_calibration 4.3.1

Armin Gabasch <[email protected]>

Please report any problems to [email protected]. Alternatively, you may send a report to the ESO User Support Department <[email protected]>.

GPL