NAME

       fors_photometry - Compute corrected flatfield

SYNOPSIS

       esorex fors_photometry [OPTIONS] FILE.sof

DESCRIPTION

       Input files:
         DO category:               Type:       Explanation:             Number:
         PHOT_TABLE                 FITS table  Expected extinction params  1
         ALIGNED_PHOT               FITS table  Photometry                  1+
         MASTER_SKY_FLAT_IMG        FITS image  Master flat field           1

       Output files:
         DO category:               Data type:  Explanation:
         PHOT_COEFF_TABLE           FITS image  Observed extinction coefficients
         CORRECTION_MAP             FITS image  Correction map (magnitude)
         CORRECTION_FACTOR          FITS image  Correction map (flux)
         MASTER_FLAT_IMG            FITS image  Corrected master flat field

OPTIONS

       --fitz <bool>
              Fit  zeropoint  (bool;  default: True). The full name of this option for the EsoRex
              configuration file is fors.fors_photometry.fitz [default = True].

       --fit_all_mag <bool>
              Always fit star magnitudes (bool; default: False). The full name of this option for
              the  EsoRex  configuration  file  is  fors.fors_photometry.fit_all_mag  [default  =
              False].

       --fite <str>
              Fit atmospheric extinctions (str; default:  ´pernight´).  The  full  name  of  this
              option  for  the  EsoRex configuration file is fors.fors_photometry.fite [default =
              pernight].

       --fitc <bool>
              Fit color correction term (bool; default: False). The full name of this option  for
              the EsoRex configuration file is fors.fors_photometry.fitc [default = False].

       --use_all_stars <bool>
              Use  also  non-standard  stars to fit polynomial f (bool; default: False). The full
              name    of    this    option    for    the    EsoRex    configuration    file    is
              fors.fors_photometry.use_all_stars [default = False].

       --degreef1 <int>
              FLatfield  correction map polynomial degree (x) (int; default: 0). The full name of
              this option for the  EsoRex  configuration  file  is  fors.fors_photometry.degreef1
              [default = 0].

       --degreef2 <int>
              Flatfield  correction  map  polynomial  degree  (y),  or  negative  for  triangular
              coefficient matrix (int; default: -1). The full name of this option for the  EsoRex
              configuration file is fors.fors_photometry.degreef2 [default = -1].

       --degreep <int>
              Extinction/color  coupling  degree  (int; default: 0). The full name of this option
              for the EsoRex configuration file is fors.fors_photometry.degreep [default = 0].

       --mjd_obs_target <float>
              MJD-OBS used to match the raw frame from which EXTINCTION_PER_NIGHT and  PHOT_COEFF
              inherit  MJD-OBS.  If  negative  theMJD-OBS  of  the first raw frame isused (float;
              default: -1.0). The full name of this option for the EsoRex configuration  file  is
              fors.fors_photometry.mjd_obs_target [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.

SEE ALSO

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

              ftp://ftp.eso.org/pub/dfs/pipelines/fors/fors-pipeline-manual-4.9.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  fors  pipeline  are  fors_align_sky(7),  fors_align_sky_lss(7),
       fors_bias(7),   fors_calib(7),   fors_config(7),   fors_dark(7),   fors_detect_objects(7),
       fors_detect_spectra(7), fors_extract(7),  fors_extract_objects(7),  fors_extract_slits(7),
       fors_flatfield(7),   fors_img_science(7),  fors_img_screen_flat(7),  fors_img_sky_flat(7),
       fors_normalise_flat(7),  fors_pmos_calib(7),  fors_pmos_extract(7),  fors_pmos_science(7),
       fors_remove_bias(7),      fors_resample(7),      fors_science(7),      fors_spec_mflat(7),
       fors_subtract_sky(7),   fors_subtract_sky_lss(7),   fors_sumflux(7),   fors_trace_flat(7),
       fors_wave_calib(7), fors_wave_calib_lss(7), fors_zeropoint(7)

VERSION

       fors_photometry 5.4.3

AUTHOR

       Jonas M. Larsen <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 currently part of  the  FORS  Instrument  Pipeline  Copyright  (C)  2002-2011
       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  02110-1301  USA