Provided by: cpl-plugin-fors-doc_4.11.12+dfsg-3_all 
NAME
fors_wave_calib_lss - Derive dispersion relation from long-slit arc lamp frame
SYNOPSIS
esorex fors_wave_calib_lss [OPTIONS] FILE.sof
DESCRIPTION
This recipe is used to wavelength calibrate one long slit spectrum, i.e., a FORS spectral
obtained either in LSS mode or in MOS/MXU mode with all slits at the same offset. A
pattern-matching algorithm is applied as in recipe fors_detect_spectra. For more details
on this data reduction strategy please refer to the FORS Pipeline User´s Manual.
Note that specifying an input GRISM_TABLE will set some of the recipe configuration
parameters to default values valid for a particular grism.
In the table below the LSS acronym can be alternatively read as MOS or MXU.
Input files:
DO category: Type: Explanation: Required:
LAMP_UNBIAS_LSS Calib Arc lamp exposure Y
MASTER_LINECAT Calib Line catalog Y
GRISM_TABLE Calib Grism table .
Output files:
DO category: Data type: Explanation:
REDUCED_LAMP_LSS FITS image Calibrated arc lamp exposure
DISP_COEFF_LSS FITS table Inverse dispersion coefficients
DISP_RESIDUALS_LSS FITS image Image of modeling residuals
WAVELENGTH_MAP_LSS FITS image Wavelengths mapped on CCD
SLIT_LOCATION_LSS FITS image Background subtracted arc frame
SPECTRAL_RESOLUTION_LSS FITS table Spectral resolution table
OPTIONS
--dispersion <float>
Expected spectral dispersion (Angstrom/pixel) (float; default: 0.0). The full name
of this option for the EsoRex configuration file is
fors.fors_wave_calib_lss.dispersion [default = 0.0].
--peakdetection <float>
Initial peak detection threshold (ADU) (float; default: 0.0). The full name of this
option for the EsoRex configuration file is fors.fors_wave_calib_lss.peakdetection
[default = 0.0].
--wdegree <long>
Degree of wavelength calibration polynomial (long; default: 0). The full name of
this option for the EsoRex configuration file is fors.fors_wave_calib_lss.wdegree
[default = 0].
--wradius <long>
Search radius if iterating pattern-matching with first-guess method (long; default:
4). The full name of this option for the EsoRex configuration file is
fors.fors_wave_calib_lss.wradius [default = 4].
--wreject <float>
Rejection threshold in dispersion relation fit (pixel) (float; default: 0.7). The
full name of this option for the EsoRex configuration file is
fors.fors_wave_calib_lss.wreject [default = 0.7].
--wcolumn <str>
Name of line catalog table column with wavelengths (str; default: ´WLEN´). The full
name of this option for the EsoRex configuration file is
fors.fors_wave_calib_lss.wcolumn [default = WLEN].
--startwavelength <float>
Start wavelength in spectral extraction (float; default: 0.0). The full name of
this option for the EsoRex configuration file is
fors.fors_wave_calib_lss.startwavelength [default = 0.0].
--endwavelength <float>
End wavelength in spectral extraction (float; default: 0.0). The full name of this
option for the EsoRex configuration file is fors.fors_wave_calib_lss.endwavelength
[default = 0.0].
--wmode <long>
Interpolation mode of wavelength solution (0 = no interpolation, 1 = fill gaps, 2 =
global model) (long; default: 2). The full name of this option for the EsoRex
configuration file is fors.fors_wave_calib_lss.wmode [default = 2].
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-4.7.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 fors pipeline are fors_img_sky_flat(7), fors_resample(7),
fors_config(7), fors_extract_objects(7), fors_calib(7), fors_wave_calib(7),
fors_detect_objects(7), fors_pmos_science(7), fors_zeropoint(7), fors_extract_slits(7),
fors_extract(7), fors_remove_bias(7), fors_subtract_sky(7), fors_normalise_flat(7),
fors_photometry(7), fors_img_screen_flat(7), fors_dark(7), fors_subtract_sky_lss(7),
fors_trace_flat(7), fors_flatfield(7), fors_img_science(7), fors_detect_spectra(7),
fors_sumflux(7), fors_pmos_extract(7), fors_align_sky_lss(7), fors_bias(7),
fors_align_sky(7), fors_pmos_calib(7), fors_spec_mflat(7), fors_science(7)
VERSION
fors_wave_calib_lss 4.11.12
AUTHOR
Carlo Izzo <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) 2002-2010
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