Provided by: cpl-plugin-visir-doc_4.3.8+dfsg-1_all bug

NAME

       visir_old_spc_wcal - Old DRS detector: Spectroscopic wavelength calibration recipe

SYNOPSIS

       esorex visir_old_spc_wcal [OPTIONS] FILE.sof

DESCRIPTION

       This  recipe estimates the dispersion relation using the atmospheric spectrum in a long-slit spectroscopy
       half-cycle frame.

       The files listed in the Set Of Frames (sof-file) must be  tagged:  VISIR-Long-Slit-Spectroscopy-file.fits
       SPEC_CAL_LMR_WCAL               VISIR-Quantum-Efficiency-Calibration-file.fits              SPEC_CAL_QEFF
       VISIR-Atmospheric-Emission-Lines-Calibration-file.fits SPEC_CAL_LINES

       Additionally, a bad pixel map with a PRO.CATG of SPEC_BPM may be added to the Set  Of  Frames  with  tag:
       BPM.

OPTIONS

       --auto_bpm <bool>
              Automatic  detection  and  correction  of  bad pixels (bool; default: True). The full name of this
              option for the EsoRex configuration file is visir.visir_old_spc_wcal.auto_bpm [default = True].

       --plot <int>
              The recipe can produce a number of predefined plots.  Zero  means  that  none  of  the  plots  are
              produced,  while  increasing  values  (e.g. 1 or 2) increases the number of plots produced. If the
              plotting fails a warning is produced, and the recipe  continues.  The  default  behaviour  of  the
              plotting  is  to  use gnuplot (with option -persist). The recipe currently produces 1D-plots using
              gnuplot commands. The recipe user can control the actual plotting-command used by  the  recipe  to
              create  the plot by setting the environment variable CPL_PLOTTER. Currently, if CPL_PLOTTER is set
              it must contain the string ´gnuplot´. Setting it to ´cat > my_gnuplot_$$.txt´ causes a  number  of
              ASCII-files to be created, which each produce a plot when given as standard input to gnuplot (e.g.
              later or on a different computer). 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) and then setting CPL_PLOTTER  to  my_gnuplot.pl.
              The  predefined plots include plotting of images. Images can be plotted not only with gnuplot, but
              also using the pnm format. This  is  controlled  with  the  environment  variable  CPL_IMAGER.  If
              CPL_IMAGER is set to a string that does not contain the word gnuplot, the recipe will generate the
              plot in pnm format. E.g.  setting CPL_IMAGER to ´display - &´  will  produce  a  gray-scale  image
              using  the  image  viewer  display. (int; default: 0). The full name of this option for the EsoRex
              configuration file is visir.visir_old_spc_wcal.plot [default = 0].

       --slit_skew <float>
              Distortion correction: Skew of slit (degrees) (clockwise) (float; default: 0.52). The full name of
              this option for the EsoRex configuration file is visir.visir_old_spc_wcal.phi [default = 0.52].

       --spectrum_skew <float>
              Distortion  correction:  LMR  Skew  of  spectrum  (degrees) (counter- clockwise). Not used in High
              Resolution (float; default: 1.73). The full name of this option for the EsoRex configuration  file
              is visir.visir_old_spc_wcal.ksi [default = 1.73].

       --vert_arc <float>
              Distortion  correction:  LR  Detector vertical curvature (pixel). Reduced by a factor 4 in MR. Not
              used in HR A-side. Increased by a factor 115/52 in HR B-side (float; default: -0.8). The full name
              of this option for the EsoRex configuration file is visir.visir_old_spc_wcal.eps [default = -0.8].

       --hori_arc <float>
              Distortion correction: LMR Detector horizontal curvature (pixel).  Increased by a factor 1.5 in HR
              A-side. Reduced by a factor 2 in HR B-side (float; default: 0.0). The full name of this option for
              the EsoRex configuration file is visir.visir_old_spc_wcal.delta [default = 0.0].

       --rl <int>
              Reject  leftmost  columns  in spectrum extraction, zero means all columns on the left are used. In
              cross-dispersion mode a (small) negative number may be used (pixel) (int; default:  0).  The  full
              name  of  this  option  for  the EsoRex configuration file is visir.visir_old_spc_wcal.reject_left
              [default = 0].

       --rr <int>
              Reject rightmost columns in spectrum extraction, zero means all columns on the right are used.  In
              cross-dispersion  mode  a  (small) negative number may be used (pixel) (int; default: 0). The full
              name of this option for the EsoRex  configuration  file  is  visir.visir_old_spc_wcal.reject_right
              [default = 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.

SEE ALSO

       The full documentation for the visir pipeline can be downloaded as a PDF file using the following URL:

              ftp://ftp.eso.org/pub/dfs/pipelines/visir/visir-pipeline-manual-1.4.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 visir  pipeline  are  visir_img_dark(7),  visir_img_ff(7),  visir_img_reduce(7),
       visir_img_trans(7),      visir_old_img_combine(7),      visir_old_img_phot(7),      visir_old_spc_obs(7),
       visir_old_spc_obs_ech(7),  visir_old_spc_phot(7),  visir_old_spc_phot_ech(7),  visir_old_spc_wcal_ech(7),
       visir_old_util_destripe(7),     visir_spc_reduce(7),    visir_util_apply_calib(7),    visir_util_clip(7),
       visir_util_convert_weight(7), visir_util_detect_shift(7), visir_util_img_std_cat(7),  visir_util_join(7),
       visir_util_qc(7),      visir_util_repack(7),      visir_util_run_swarp(7),     visir_util_spc_std_cat(7),
       visir_util_spc_txt2fits(7), visir_util_undistort(7)

VERSION

       visir_old_spc_wcal 4.3.8

AUTHOR

       Lars Lundin <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 part of the VISIR Instrument Pipeline Copyright (C) 2004, 2005 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