Remove crhs from an image
esorex uves_utl_remove_crh_single [OPTIONS] FILE.sof
This recipe performs image computation.
The input files is one image their associated tags should be IMA.
The output is the image cleaned from CRHs Information on relevant parameters can be found with esorex --params uves_utl_remove_crh_single esorex --help uves_utl_remove_crh_single
--crh_frac_max <float>
Maximum fraction of allowed CRHs (float; default: 0.7). The full name of this option for the EsoRex configuration file is uves.uves_utl_remove_crh_single.crh_frac_max [default = 0.7].
--sigma_lim <float>
Maximum sigma in kappa-sigma clip (float; default: 25.0). The full name of this option for the EsoRex configuration file is uves.uves_utl_remove_crh_single.sigma_lim [default = 25.0].
--f_lim <float>
Max fraction of bad pixels allowed (float; default: 0.7). The full name of this option for the EsoRex configuration file is uves.uves_utl_remove_crh_single.f_lim [default = 0.7].
--max_iter <long>
Max fraction of bad pixels allowed (long; default: 5). The full name of this option for the EsoRex configuration file is uves.uves_utl_remove_crh_single.max_iter [default = 5].
--gain <float>
Detector\'s gain (float; default: 2.42). The full name of this option for the EsoRex configuration file is uves.uves_utl_remove_crh_single.gain [default = 2.42].
--ron <float>
Detector\'s ron (float; default: 1.0). The full name of this option for the EsoRex configuration file is uves.uves_utl_remove_crh_single.ron [default = 1.0].
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 uves pipeline can be downloaded as a PDF file using the following URL:
ftp://ftp.eso.org/pub/dfs/pipelines/uves/uves-pipeline-manual-5.4.3.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 uves pipeline are uves_cal_response(7), uves_cal_mflat_combine(7), flames_utl_unpack(7), flames_cal_wavecal(7), uves_cal_mkmaster(7), flames_obs_redchain(7), uves_cal_wavecal(7), uves_cal_tflat(7), uves_cal_mflat(7), flames_cal_prep_sff_ofpos(7), uves_obs_scired(7), uves_cal_mbias(7), uves_utl_ima_arith(7), flames_obs_scired(7), uves_cal_orderpos(7), flames_cal_mkmaster(7), flames_cal_predict(7), uves_cal_mdark(7), uves_cal_cd_align(7), uves_obs_redchain(7), flames_cal_orderpos(7), uves_cal_predict(7)
uves_utl_remove_crh_single 5.4.3
Andrea Modigliani <[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 part of the ESO UVES Instrument Pipeline Copyright (C) 2004,2005,2006 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, 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA