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UVES_CAL_MBIAS(7) uves recipes UVES_CAL_MBIAS(7)

NAME

uves_cal_mbias - Creates the master bias frame

SYNOPSIS

esorex uves_cal_mbias [OPTIONS] FILE.sof

DESCRIPTION

This recipe creates a master bias frame by computing the median of all input bias frames. All input frames must have same tag and size and must be either BIAS_BLUE or BIAS_RED.

On blue input the recipe computes one master bias frame; on red input a master bias frame for each chip is produced. The average, standard deviation and median of the master bias image(s) are written to the FITS header(s)

OPTIONS

Clean detector traps. If TRUE detector traps are interpolated.The bad pixels are replaced by the average of thenearest good pixels in the same column, or simply marked as bad. The positions of bad pixels are hard-coded (as function of UVES chip). (bool; default: False). The full name of this option for the EsoRex configuration file is uves_cal_mbias.clean_traps [default = False].
x-size (pixel) of the mask starting at (x,y) = (1,1) (int; default: 1). The full name of this option for the EsoRex configuration file is uves_cal_mbias.dc_mask_x [default = 1].
y-size (pixel) of the mask starting at (x,y) = (1,1) (int; default: 1). The full name of this option for the EsoRex configuration file is uves_cal_mbias.dc_mask_y [default = 1].
Whether or not to save intermediate results to local directory (bool; default: False). The full name of this option for the EsoRex configuration file is uves.debug [default = False].
Kappa used to clip high level values, when method is set to ´mean´ (float; default: 5.0). The full name of this option for the EsoRex configuration file is uves_cal_mbias.khigh [default = 5.0].
Kappa used to clip low level values, when method is set to ´mean´ (float; default: 5.0). The full name of this option for the EsoRex configuration file is uves_cal_mbias.klow [default = 5.0].
Number of kappa sigma iterations, when method is set to ´mean´ (int; default: 5). The full name of this option for the EsoRex configuration file is uves_cal_mbias.niter [default = 5].
Determine Fixed Pattern Noise. If TRUE the Fixed Patter Noise power spectrum is determined.(as function of UVES chip). (bool; default: False). The full name of this option for the EsoRex configuration file is uves_cal_mbias.pd_compute [default = False].
Any plots produced by the recipe are redirected to the command specified by this parameter. The plotting command must contain the substring ´gnuplot´ and must be able to parse gnuplot syntax on its standard input. Valid examples of such a command may include ´gnuplot -persist´ and ´cat > mygnuplot$$.gp´. A finer control of the plotting options can be obtained by writing an executable script, e.g. my_gnuplot.pl, that executes gnuplot after setting the desired gnuplot options (e.g. set terminal pslatex color). To turn off plotting, set this parameter to ´no´ (str; default: ´no´). The full name of this option for the EsoRex configuration file is uves.plotter [default = no].
For RED arm data process the redl, redu, or both chip(s) (str; default: ´both´). The full name of this option for the EsoRex configuration file is uves.process_chip [default = both].
Method used to build master frame (str; default: ´median´). The full name of this option for the EsoRex configuration file is uves_cal_mbias.stack_method [default = median].

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 uves pipeline can be downloaded as a PDF file using the following URL:

ftp://ftp.eso.org/pub/dfs/pipelines/uves/uves-pipeline-manual-6.1.3.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 uves pipeline are flames_cal_mkmaster(7), flames_cal_orderpos(7), flames_cal_predict(7), flames_cal_prep_sff_ofpos(7), flames_cal_wavecal(7), flames_obs_redchain(7), flames_obs_scired(7), flames_utl_unpack(7), uves_cal_cd_align(7), uves_cal_mdark(7), uves_cal_mflat(7), uves_cal_mflat_combine(7), uves_cal_mkmaster(7), uves_cal_orderpos(7), uves_cal_predict(7), uves_cal_response(7), uves_cal_tflat(7), uves_cal_wavecal(7), uves_obs_redchain(7), uves_obs_scired(7), uves_utl_ima_arith(7), uves_utl_remove_crh_single(7)

VERSION

uves_cal_mbias 6.1.3

AUTHOR

Jonas M. Larsen <cpl@eso.org>

BUG REPORTS

Please report any problems to cpl@eso.org. Alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>.

LICENSE

This file is part of the FLAMES/UVES Pipeline Copyright (C) 2004, 2005, 2006, 2007 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 02111-1307 USA

6.1.3 uves_cal_mbias