xenial (7) kmo_noise_map.7.gz

Provided by: cpl-plugin-kmos-doc_1.3.17+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_check(7),   kmo_fits_strip(7),   kmo_illumination_flat(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_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 1.3.17

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