NAME¶amber_calibrate - AMBER Derives calibrated visibilities
SYNOPSIS¶esorex amber_calibrate [OPTIONS] FILE.sof
DESCRIPTION¶This recipe calculates calibrated squared visibilities and closure phases
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
OPTIONS¶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.
SEE ALSO¶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 https://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 https://packages.python.org/python-cpl/index.html for further information.
The other recipes of the amber pipeline are amber_BeamPos(7), amber_SciCal(7), amber_ascii_export(7), amber_detector(7), amber_oimerge(7), amber_p2vm(7), amber_raw_to_fitsimage(7), amber_selector(7), amber_spectral_calibration(7), amber_trf(7)
AUTHOR¶Armin Gabasch <firstname.lastname@example.org>
BUG REPORTS¶Please report any problems to email@example.com. Alternatively, you may send a report to the ESO User Support Department <firstname.lastname@example.org>.