Provided by: cpl-plugin-muse-doc_1.2.1+dfsg-2_all 
NAME
muse_scipost_make_cube - Make a MUSE cube from a MUSE pixel table.
SYNOPSIS
esorex muse_scipost_make_cube [OPTIONS] FILE.sof
DESCRIPTION
This recipe takes a pixel table and resamples it to either a FITS cube or a Euro3D table
and optionally to a stacked spectrum. This is a part of the muse_scipost recipe.
OPTIONS
--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_scipost_make_cube.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_scipost_make_cube.lambdamax [default = 10000.0].
--resample <str>
The resampling technique to use for the final output cube. (str; default:
´drizzle´). The full name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.resample [default = drizzle].
--dx <float>
Horizontal step size for resampling (in arcsec or pixel). The following defaults
are taken when this value is set to 0.0: 0.2´´ for WFM, 0.075´´ for NFM, 1.0 if
data is in pixel units. (float; default: 0.0). The full name of this option for the
EsoRex configuration file is muse.muse_scipost_make_cube.dx [default = 0.0].
--dy <float>
Vertical step size for resampling (in arcsec or pixel). The following defaults are
taken when this value is set to 0.0: 0.2´´ for WFM, 0.075´´ for NFM, 1.0 if data is
in pixel units. (float; default: 0.0). The full name of this option for the EsoRex
configuration file is muse.muse_scipost_make_cube.dy [default = 0.0].
--dlambda <float>
Wavelength step size (in Angstrom). Natural instrument sampling is used, if this is
0.0 (float; default: 0.0). The full name of this option for the EsoRex
configuration file is muse.muse_scipost_make_cube.dlambda [default = 0.0].
--crtype <str>
Type of statistics used for detection of cosmic rays during final resampling.
"iraf" uses the variance information, "mean" uses standard (mean/stdev) statistics,
"median" uses median and the median median of the absolute median deviation. (str;
default: ´median´). The full name of this option for the EsoRex configuration file
is muse.muse_scipost_make_cube.crtype [default = median].
--crsigma <float>
Sigma rejection factor to use for cosmic ray rejection during final resampling. A
zero or negative value switches cosmic ray rejection off. (float; default: 15.0).
The full name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.crsigma [default = 15.0].
--rc <float>
Critical radius for the "renka" resampling method. (float; default: 1.25). The full
name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.rc [default = 1.25].
--pixfrac <float>
Pixel down-scaling factor for the "drizzle" resampling method. (float; default:
0.8). The full name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.pixfrac [default = 0.8].
--ld <long>
Number of adjacent pixels to take into account during resampling in all three
directions (loop distance); this affects all resampling methods except "nearest".
(long; default: 1). The full name of this option for the EsoRex configuration file
is muse.muse_scipost_make_cube.ld [default = 1].
--format <str>
Type of output file format, "Cube" is a standard FITS cube with NAXIS=3 and
multiple extensions (for data and variance). The extended "x" formats include the
reconstructed image(s) in FITS image extensions within the same file. (str;
default: ´Cube´). The full name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.format [default = Cube].
--stacked <bool>
If true, write an additional output file in form of a 2D stacked image (x direction
is pseudo-spatial, y direction is wavelength). (bool; default: False). The full
name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.stacked [default = False].
--filter <str>
The filter name(s) to be used for the output field-of-view image. Each name has to
correspond to an EXTNAME in an extension of the FILTER_LIST file. If an unsupported
filter name is given, creation of the respective image is omitted. If multiple
filter names are given, they have to be comma separated. (str; default: ´white´).
The full name of this option for the EsoRex configuration file is
muse.muse_scipost_make_cube.filter [default = white].
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_astrometry(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_subtract_sky(7),
muse_scipost_subtract_sky_simple(7), muse_standard(7), muse_twilight(7), muse_wavecal(7)
VERSION
muse_scipost_make_cube 1.2.1
AUTHOR
Ole Streicher <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