Provided by: cpl-plugin-kmos-doc_1.4.3+dfsg-1_all bug

NAME

       kmo_noise_map - Generate a noise map from a raw frame

SYNOPSIS

       esorex kmo_noise_map [OPTIONS] FILE.sof

DESCRIPTION

       The noise in each pixel of the input data is estimated using gain and readnoise.

       The  readnoise  is  expected to be in the primary header (ESO DET CHIP RON), the gain (ESO
       DET CHIP GAIN) has to be in each of the subsequent headers of  each  detector  frame.  The
       output is the initial noise map of the data frame.

         Input files:

          DO                    KMOS
          category              Type   Explanation                    Required #Frames
          --------              -----  -----------                    -------- -------
          <none or any>         RAW    raw data frame                     Y       1

         Output files:

          DO                    KMOS
          category              Type   Explanation
          --------              -----  -----------
          NOISE_MAP             F2D    Initial noise map
                                       (6 Extensions, 3 data and 3 noise)

OPTIONS

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

              ftp://ftp.eso.org/pub/dfs/pipelines/kmos/kmos-pipeline-manual-2.9.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   kmos   pipeline   are   kmo_arithmetic(7),   kmo_copy(7),
       kmo_fit_profile(7),  kmo_fits_strip(7),  kmo_make_image(7),  kmo_rotate(7),  kmo_shift(7),
       kmo_sky_mask(7),  kmo_stats(7),   kmos_combine(7),   kmos_dark(7),   kmos_extract_spec(7),
       kmos_flat(7),     kmos_gen_reflines(7),     kmos_gen_telluric(7),    kmos_illumination(7),
       kmos_reconstruct(7), kmos_sci_red(7), kmos_sky_tweak(7),  kmos_std_star(7),  kmos_test(7),
       kmos_wave_cal(7)

VERSION

       kmo_noise_map 1.4.3

AUTHOR

       Alex Agudo Berbel <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 CRIRES  Instrument  Pipeline  Copyright  (C)  2002,2003  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., 59 Temple Place, Suite  330,  Boston,
       MA  02111-1307  USA