Provided by: cpl-plugin-amber-doc_4.3.8+dfsg-1build2_all
amber_calibrate - 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-4.3.8.pdf 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)
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>.