Compute the master bias frame
esorex fors_bias [OPTIONS] FILE.sof
This recipe is used to combine input raw BIAS frames into a master bias frame. The overscan regions, if present, are removed from the result.
Input files:
DO category: Type: Explanation: Required: BIAS Raw Bias frame Y
Output files:
DO category: Data type: Explanation: MASTER_BIAS FITS image Master bias frame
--stack_method <str>
Frames combination method (str; default: \'minmax\'). The full name of this option for the EsoRex configuration file is fors.fors_bias.stack_method [default = minmax].
--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_bias.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_bias.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_bias.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_bias.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_bias.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.
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-4.9.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_extract_slits(7), test_hough(7), fors_img_screen_flat(7), fors_extract(7), fors_remove_bias(7), fors_subtract_sky(7), fors_normalise_flat(7), montecarlo(7), fors_photometry(7), fors_zeropoint(7), fors_dark(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_align_sky(7), fors_pmos_calib(7), fors_spec_mflat(7), fors_science(7)
fors_bias 5.0.0
Jonas M. Larsen, Carlo Izzo <[email protected]>
Please report any problems to [email protected]. Alternatively, you may send a report to the ESO User Support Department <[email protected]>.
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