vmifucalib(7)


NAME

   vmifucalib  - Generate IFU calibrations from a set of flat and arc lamp
   exposures.

SYNOPSIS

   esorex vmifucalib [OPTIONS] FILE.sof

DESCRIPTION

   This recipe produces the extraction mask, the  wavelength  calibration,
   and  the relative transmission correction, from a set of flat field and
   one arc lamp exposures (IFU mode).

   Input files:

     DO category:                 Type:       Explanation:       Required:
     IFU_SCREEN_FLAT              Raw         Flat field            Y
     IFU_ARC_SPECTRUM             Raw         Arc spectrum          .

     LINE_CATALOG                 Calib       Arc line catalog      .

     MASTER_BIAS                  Calib       Master bias           Y
     IFU_IDENT                    Calib       Fiber identification  .

     CCD_TABLE                    Calib       Bad pixel table       .

   Output files:

     DO category:                 Data type:  Explanation:
     IFU_MASTER_SCREEN_FLAT       FITS image  Stack of all raw flat fields
     IFU_ARC_SPECTRUM_EXTRACTED   FITS image  Extracted arc spectra
     IFU_FLAT_SPECTRUM_EXTRACTED  FITS image  Extracted flat field spectra
     IFU_TRACE                    FITS table  Extraction mask
     IFU_IDS                      FITS table  Wavelength calibration
     IFU_TRANSMISSION             FITS table  Transmission correction

   An arc spectrum exposure may not be specified in  input,  but  in  that
   case   no   wavelength  calibration  nor  fiber  relative  transmission
   correction will  be  computed,  and  further  reduction  of  associated
   scientific  data  will  not be possible; the only products in this case
   will be the stack of all the input raw flat field  exposures,  and  the
   extraction  mask.  If  the arc spectrum exposure is specified in input,
   then also a line catalog must be given. The fiber identification table,
   if  given,  ensures  that  all  spectra  will  be safely identified and
   assigned to the correct spatial position, but in most cases it will  be
   possible  to  reduce the data even without specifying this table in the
   input SOF. A CCD table must be specified only if a bad  pixel  cleaning
   is requested.

   For more details, please refer to the VIMOS Pipeline Users Guide.

OPTIONS

   --AllowSingleFrames <bool>
          Flat  fields  combination  method  is  ignored.  (bool; default:
          True). The full name of this option for the EsoRex configuration
          file is vimos.Parameters.stacking.singleframes [default = True].

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

   --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: 0). The  full  name  of  this  option  for  the  EsoRex
          configuration  file  is vimos.Parameters.stacking.minmax.minimum
          [default = 0].

   --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].

   --BiasMethod <str>
          Bias removal method. (str; default: Zmaster). The full name of
          this   option   for   the   EsoRex   configuration    file    is
          vimos.Parameters.bias.removing.method [default = Zmaster].

   --CleanBadPixel <bool>
          Bad  pixel  correction  on  master  flat  field. (bool; default:
          False).  The  full  name  of  this   option   for   the   EsoRex
          configuration file is vimos.Parameters.badpixel.clean [default =
          False].

   --ApplyTransmission <bool>
          Apply transmission correction  to  extracted  arc  lamp  spectra
          (bool;  default:  True).  The  full  name of this option for the
          EsoRex configuration file is vimos.Parameters.apply.transmission
          [default = True].

   --MaxIdsRms <float>
          Maximum  tolerated  RMS of residuals in IDS fit (float; default:
          2.0). The full name of this option for the EsoRex  configuration
          file is vimos.Parameters.ids.maxrms [default = 2.0].

   --LineIdent <str>
          Arc  line  identification  method.  (str; default: Blind). The
          full name of this option for the EsoRex  configuration  file  is
          vimos.Parameters.line.ident.method [default = Blind].

   --MaxTraceRejection <long>
          Maximum  percentage  of  rejected  positions  in  fiber  spectra
          tracing (long; default: 33). The full name of  this  option  for
          the  EsoRex  configuration file is vimos.Parameters.trace.failed
          [default = 33].

   --ComputeQC <bool>
          Compute QC1 parameters (bool; default: True). The full  name  of
          this    option    for   the   EsoRex   configuration   file   is
          vimos.Parameters.quality.enable [default = True].

   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),    vmifucombine(7),   vmifucombinecube(7),   vmifuscience(7),
   vmifustandard(7),  vmimcalphot(7),  vmimflatscreen(7),  vmimflatsky(7),
   vmimobsjitter(7),  vmimobsstare(7), vmimpreimaging(7), vmimstandard(7),
   vmmoscalib(7),  vmmoscombine(7),  vmmosobsjitter(7),  vmmosobsstare(7),
   vmmosscience(7),    vmmosstandard(7),    vmspcaldisp(7),   vmspflat(7),
   vmspphot(7)

VERSION

   vmifucalib 3.1.7

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 currently part of the VIMOS 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





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