xenial (7) vmmoscombine.7.gz

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NAME

       vmmoscombine - Combine reduced MOS observations from different OBs.

SYNOPSIS

       esorex vmmoscombine [OPTIONS] FILE.sof

DESCRIPTION

       This  recipe  is used to sum the contributes from a sequence of 2D-extracted spectral frames generated by
       the recipes vmmosobsstare, vmmosobsjitter, and vmmoscombine itself. The  only  restriction  is  that  all
       frames  must  be  obtained with the same mask. Sky subtraction, fringing correction, flat fielding, etc.,
       are not applied, since they had been applied in the previous reduction of each input dataset.

       Each input image is corrected to airmass zero before the stacking, and for  this  reason  an  atmospheric
       extinction  table  must always be specified. Optionally a correction for the instrument response can also
       be applied.

       Input files:

         DO category:             Type:       Explanation:          Required:
         MOS_SCIENCE_EXTRACTED    Product     Combined slit spectra     Y
         GRISM_TABLE              Calib       Grism table               Y
         EXTINCT_TABLE            Calib       Atmospheric extinction    Y
         MOS_SPECPHOT_TABLE       Calib       Response curve            .

       Output files:

         DO category:             Data type:  Explanation:
         MOS_SCIENCE_REDUCED      FITS image  Extracted objects spectra
         MOS_SCIENCE_FLUX_REDUCED FITS image  Flux calibrated objects spectra
         MOS_SCIENCE_EXTRACTED    FITS image  Combined slit spectra
         OBJECT_TABLE             FITS table  Objects spectra identification
         WINDOW_TABLE             FITS table  Objects positions in slit

       The positions of the extracted slit spectra and of the detected objects that they may contain are  listed
       in the window table.

       If a spectro-photometric table (produced by the recipe vmmosstandard) is specified and a flux calibration
       is requested, then a MOS_SCIENCE_FLUX_REDUCED image is also created.  This  image  is  identical  to  the
       MOS_SCIENCE_REDUCED,  but  the  spectra  it  contains  are  flux  calibrated,  and  expressed in units of
       erg/cm/cm/s/Angstrom.

       For more details, please refer to the VIMOS Pipeline User´s Guide.

OPTIONS

       --StackMethod <str>
              Frames combination method (str; default: ´Average´). The full name of this option for  the  EsoRex
              configuration file is vimos.Parameters.stacking.method [default = Average].

       --KSigmaLow <float>
              Low threshold for K-sigma clipping method. (float; default: 5.0). The full name of this option for
              the EsoRex configuration file is vimos.Parameters.stacking.ksigma.low [default = 5.0].

       --KSigmaHigh <float>
              High threshold for K-sigma clipping method. (float; default: 5.0). The full name  of  this  option
              for the EsoRex configuration file is vimos.Parameters.stacking.ksigma.high [default = 5.0].

       --MinRejection <long>
              Number  of  lowest rejected values for rejection method. (long; default: 1). The full name of this
              option for the EsoRex configuration file is  vimos.Parameters.stacking.minmax.minimum  [default  =
              1].

       --MaxRejection <long>
              Number  of highest rejected values for rejection method. (long; default: 1). The full name of this
              option for the EsoRex configuration file is  vimos.Parameters.stacking.minmax.maximum  [default  =
              1].

       --DetectionLevel <float>
              Object  detection level in units of sigma. (float; default: 2.0). The full name of this option for
              the EsoRex configuration file is vimos.Parameters.detection.sigma [default = 2.0].

       --WatershedLevels <long>
              Number of levels in the watershed method in object detection. (long; default: 32). The  full  name
              of  this  option for the EsoRex configuration file is vimos.Parameters.detection.levels [default =
              32].

       --WatershedFraction <float>
              Flux fraction to use in watershed. (float; default: 0.01). The full name of this  option  for  the
              EsoRex configuration file is vimos.Parameters.detection.fraction [default = 0.01].

       --MinObjectSize <long>
              Minimal  size  for  an  object candidate to be considered an object.  (long; default: 2). The full
              name of this option  for  the  EsoRex  configuration  file  is  vimos.Parameters.detection.minsize
              [default = 2].

       --MaxObjectSize <long>
              Maximal size for an object candidate for not trying deblend into sub- objects. (long; default: 7).
              The    full    name    of    this    option    for    the    EsoRex    configuration    file    is
              vimos.Parameters.detection.maxsize [default = 7].

       --CalibrateFlux <bool>
              Extracted  spectra  are  flux calibrated. (bool; default: False). The full name of this option for
              the EsoRex configuration file is vimos.Parameters.flux.calibration [default = False].

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

              ftp://ftp.eso.org/pub/dfs/pipelines/vimos/vimos-pipeline-manual-6.9.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  vimos  pipeline  are  vmbias(7),  vmdark(7),  vmdet(7),  vmifucalib(7),
       vmifucombine(7),     vmifucombinecube(7),     vmifuscience(7),     vmifustandard(7),      vmimcalphot(7),
       vmimflatscreen(7), vmimflatsky(7), vmimobsjitter(7), vmimobsstare(7), vmimpreimaging(7), vmimstandard(7),
       vmmoscalib(7), vmmosobsjitter(7), vmmosobsstare(7),  vmmosscience(7),  vmmosstandard(7),  vmspcaldisp(7),
       vmspflat(7), vmspphot(7)

VERSION

       vmmoscombine 3.0.6

AUTHOR

       ESO VIMOS Pipeline Team and VIMOS Consortium <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 VIMOS Instrument Pipeline Copyright (C) 2002-2005 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  02110-1301 USA