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NAME

       muse_astrometry - Compute an astrometric solution.

SYNOPSIS

       esorex muse_astrometry [OPTIONS] FILE.sof

DESCRIPTION

       Merge   pixel  tables  from  all  IFUs,  apply  correction  for  differential  atmospheric
       refraction, optionally apply flux calibration and telluric correction  (if  the  necessary
       input  data  was given), and resample the data from all exposures into a datacube. Use the
       cube to detect objects which are then matched to their reference positions  from  which  a
       two-dimensional WCS solution is computed. The main output is the ASTROMETRY_WCS file which
       is a bare FITS header containing the world coordinate solution. The secondary  product  is
       DATACUBE_ASTROMETRY,  it  is  not  needed  for  further  processing  but  can  be used for
       verification and debugging. It contains the reconstructed cube and two images created from
       it  in further FITS extensions: a white-light image and the special image created from the
       central planes of the cube used  to  detect  and  centroid  the  stars  (as  well  as  its
       variance).

OPTIONS

       --centroid <str>
              Centroiding method to use for objects in the field of view. "gaussian" and "moffat"
              use 2D fits to derive the centroid, "box" is a simple centroid  in  a  square  box.
              (str; default: ´moffat´). The full name of this option for the EsoRex configuration
              file is muse.muse_astrometry.centroid [default = moffat].

       --detsigma <float>
              Source detection sigma level to use. (float; default: 3.0). The full name  of  this
              option  for the EsoRex configuration file is muse.muse_astrometry.detsigma [default
              = 3.0].

       --radius <float>
              Initial radius in pixels for pattern matching  identification  in  the  astrometric
              field.  (float;  default:  5.0).  The  full  name  of  this  option  for the EsoRex
              configuration file is muse.muse_astrometry.radius [default = 5.0].

       --faccuracy <float>
              Factor of initial accuracy relative to mean positional  accuracy  of  the  measured
              positions to use for pattern matching. (float; default: 5.0). The full name of this
              option for the EsoRex configuration file is muse.muse_astrometry.faccuracy [default
              = 5.0].

       --niter <long>
              Number  of  iterations of the astrometric fit. (long; default: 2). The full name of
              this  option  for  the  EsoRex  configuration  file  is  muse.muse_astrometry.niter
              [default = 2].

       --rejsigma <float>
              Rejection  sigma level of the astrometric fit. (float; default: 3.0). The full name
              of this option for the EsoRex configuration file  is  muse.muse_astrometry.rejsigma
              [default = 3.0].

       --rotcenter <str>
              Center  of  rotation of the instrument, given as two comma-separated floating point
              values in pixels. (str; default: ´-0.01,-1.20´). The full name of this  option  for
              the   EsoRex   configuration  file  is  muse.muse_astrometry.rotcenter  [default  =
              -0.01,-1.20].

       --lambdamin <float>
              Cut off the data below this wavelength after loading the  pixel  table(s).  (float;
              default: 4000.0). The full name of this option for the EsoRex configuration file is
              muse.muse_astrometry.lambdamin [default = 4000.0].

       --lambdamax <float>
              Cut off the data above this wavelength after loading the  pixel  table(s).  (float;
              default:  10000.0).  The full name of this option for the EsoRex configuration file
              is muse.muse_astrometry.lambdamax [default = 10000.0].

       --lambdaref <float>
              Reference wavelength used for correction of  differential  atmospheric  refraction.
              The  R-band  (peak  wavelength ~7000 Angstrom) that is usually used for guiding, is
              close to the central wavelength of MUSE, so a value of 7000.0  Angstrom  should  be
              used if nothing else is known.  A value less than zero switches DAR correction off.
              (float; default: 7000.0). The full name of this option for the EsoRex configuration
              file is muse.muse_astrometry.lambdaref [default = 7000.0].

       --darcheck <str>
              Carry  out  a  check of the theoretical DAR correction using source centroiding. If
              "correct" it will also apply an empirical correction.  (str; default: ´none´).  The
              full    name    of   this   option   for   the   EsoRex   configuration   file   is
              muse.muse_astrometry.darcheck [default = none].

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

              ftp://ftp.eso.org/pub/dfs/pipelines/muse/muse-pipeline-cookbook-1.2.1.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 muse pipeline are muse_ampl(7), muse_bias(7), muse_create_sky(7),
       muse_dark(7),  muse_exp_align(7),  muse_exp_combine(7),  muse_flat(7),   muse_geometry(7),
       muse_lsf(7),          muse_qi_mask(7),          muse_scibasic(7),         muse_scipost(7),
       muse_scipost_apply_astrometry(7),                          muse_scipost_calibrate_flux(7),
       muse_scipost_combine_pixtables(7),                            muse_scipost_correct_dar(7),
       muse_scipost_correct_rv(7),    muse_scipost_make_cube(7),    muse_scipost_subtract_sky(7),
       muse_scipost_subtract_sky_simple(7), muse_standard(7), muse_twilight(7), muse_wavecal(7)

VERSION

       muse_astrometry 1.2.1

AUTHOR

       Peter Weilbacher <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 MUSE  Instrument  Pipeline  Copyright  (C)  2005,  2015  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  02111-1307  USA