Amber derives calibrated visibilities
esorex amber_calibrate [OPTIONS] FILE.sof
This recipe calculates calibrated squared visibilities and closure phases
Input files:
DO category: Type: Explanation: Required: SCIENCE_REDUCED Products Science frame or Y SCIENCE_REDUCED_FILTERED Products Science frame
AMBER_TRF_J Calib J-Band transfer function and/or AMBER_TRF_H Calib H-Band transfer function Y and/or AMBER_TRF_K Calib K-Band transfer function
Output files:
DO category: Data type: Explanation: SCIENCE_CALIBRATED calibrated (vis2) OI-fits file
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_raw_to_fitsimage(7), amber_p2vm(7), amber_BeamPos(7), amber_detector(7), amber_oimerge(7), amber_SciCal(7), amber_trf(7), amber_spectral_calibration(7), amber_selector(7), amber_ascii_export(7)
amber_calibrate 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