NAME

       muse_scipost_raman - Remove of 4GLSF Raman emission.

SYNOPSIS

       esorex muse_scipost_raman [OPTIONS] FILE.sof

DESCRIPTION

       This  recipe  removes  the Raman scattered light of the 4GLSF system from the exposure. It
       must be before the normal sky subtraction.

OPTIONS

       --lambdamin <float>
              Cut off the data below this wavelength after loading the  pixel  table(s).  (float;
              default: 4000.0). The full name of this option for the EsoRex configuration file is
              muse.muse_scipost_raman.lambdamin [default = 4000.0].

       --lambdamax <float>
              Cut off the data above this wavelength after loading the  pixel  table(s).  (float;
              default:  10000.0).  The full name of this option for the EsoRex configuration file
              is muse.muse_scipost_raman.lambdamax [default = 10000.0].

       --lambdaref <float>
              Reference wavelength used for correction of  differential  atmospheric  refraction.
              The  R-band  (peak  wavelength ~7000 Angstrom) that is usually used for guiding, is
              close to the central wavelength of MUSE, so a value of 7000.0  Angstrom  should  be
              used if nothing else is known.  A value less than zero switches DAR correction off.
              (float; default: 7000.0). The full name of this option for the EsoRex configuration
              file is muse.muse_scipost_raman.lambdaref [default = 7000.0].

       --width <float>
              Wavelength  range  around  Raman lines [Angstrom]. (float; default: 20.0). The full
              name    of    this    option    for    the    EsoRex    configuration    file    is
              muse.muse_scipost_raman.width [default = 20.0].

       --crsigma <float>
              Sigma   level   clipping   for   cube-based   CR  rejection  (using  "median",  see
              muse_scipost). It can be switched off, by passing zero or a negative value. (float;
              default:  15.0).  The full name of this option for the EsoRex configuration file is
              muse.muse_scipost_raman.crsigma [default = 15.0].

       --fraction <float>
              Fraction of the image (without the ignored part) to be considered  as  sky.  If  an
              input sky mask is provided, the fraction is applied to the regions within the mask.
              If the whole sky mask should be used, set this parameter  to  1.  (float;  default:
              0.75).  The  full  name  of  this  option  for  the  EsoRex  configuration  file is
              muse.muse_scipost_raman.fraction [default = 0.75].

       --ignore <float>
              Lowest fraction of the image to be ignored. If an input sky mask is  provided,  the
              fraction is applied to the regions within the mask. If the whole sky mask should be
              used, set this parameter to 0. (float; default: 0.05). The full name of this option
              for  the  EsoRex  configuration  file  is muse.muse_scipost_raman.ignore [default =
              0.05].

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

              ftp://ftp.eso.org/pub/dfs/pipelines/muse/muse-pipeline-cookbook-2.8.5.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 muse pipeline are muse_ampl(7), muse_astrometry(7), muse_bias(7),
       muse_create_sky(7), muse_dark(7),  muse_exp_align(7),  muse_exp_combine(7),  muse_flat(7),
       muse_geometry(7),    muse_illum(7),    muse_lingain(7),    muse_lsf(7),   muse_qi_mask(7),
       muse_scibasic(7),            muse_scipost(7),            muse_scipost_apply_astrometry(7),
       muse_scipost_calibrate_flux(7),                         muse_scipost_combine_pixtables(7),
       muse_scipost_correct_dar(7),    muse_scipost_correct_rv(7),     muse_scipost_make_cube(7),
       muse_scipost_subtract_sky(7),    muse_scipost_subtract_sky_simple(7),    muse_standard(7),
       muse_twilight(7), muse_wavecal(7)

VERSION

       muse_scipost_raman 2.8.5

AUTHOR

       Ole Streicher <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  MUSE  Instrument Pipeline Copyright (C) 2005, 2019 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