Provided by: cpl-plugin-fors-doc_4.11.12+dfsg-3_all
NAME
fors_dark - Compute master dark frame
SYNOPSIS
esorex fors_dark [OPTIONS] FILE.sof
DESCRIPTION
This recipe is used to combine input raw DARK frames into a master dark frame by subtracing the master bias and using the given stacking method. The overscan regions, if present, are removed from the result. Input files: DO category: Type: Explanation: Required: DARK Raw Dark frame Y MASTER_BIAS FITS image Master bias Y Output files: DO category: Data type: Explanation: MASTER_DARK FITS image Master dark frame
OPTIONS
--stack_method <str> Frames combination method (str; default: ´median´). The full name of this option for the EsoRex configuration file is fors.fors_dark.stack_method [default = median]. --minrejection <long> Number of lowest values to be rejected (long; default: 1). The full name of this option for the EsoRex configuration file is fors.fors_dark.minrejection [default = 1]. --maxrejection <long> Number of highest values to be rejected (long; default: 1). The full name of this option for the EsoRex configuration file is fors.fors_dark.maxrejection [default = 1]. --klow <float> Low threshold in ksigma method (float; default: 3.0). The full name of this option for the EsoRex configuration file is fors.fors_dark.klow [default = 3.0]. --khigh <float> High threshold in ksigma method (float; default: 3.0). The full name of this option for the EsoRex configuration file is fors.fors_dark.khigh [default = 3.0]. --kiter <long> Max number of iterations in ksigma method (long; default: 999). The full name of this option for the EsoRex configuration file is fors.fors_dark.kiter [default = 999]. 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 fors pipeline can be downloaded as a PDF file using the following URL: ftp://ftp.eso.org/pub/dfs/pipelines/fors/fors-pipeline-manual-4.7.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 fors pipeline are fors_wave_calib_lss(7), fors_img_sky_flat(7), fors_resample(7), fors_config(7), fors_extract_objects(7), fors_calib(7), fors_wave_calib(7), fors_detect_objects(7), fors_pmos_science(7), fors_zeropoint(7), fors_extract_slits(7), fors_extract(7), fors_remove_bias(7), fors_subtract_sky(7), fors_normalise_flat(7), fors_photometry(7), fors_img_screen_flat(7), fors_subtract_sky_lss(7), fors_trace_flat(7), fors_flatfield(7), fors_img_science(7), fors_detect_spectra(7), fors_sumflux(7), fors_pmos_extract(7), fors_align_sky_lss(7), fors_bias(7), fors_align_sky(7), fors_pmos_calib(7), fors_spec_mflat(7), fors_science(7)
VERSION
fors_dark 4.11.12
AUTHOR
Jonas M. Larsen <usd-help@eso.org>
BUG REPORTS
Please report any problems to usd-help@eso.org. Alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>.
LICENSE
This file is currently part of the FORS Instrument Pipeline Copyright (C) 2002-2011 European Southern Observatory This program is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version. This program is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with this program; if not, write to the Free Software Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA 02110-1301 USA