Provided by: cpl-plugin-kmos-doc_2.1.0+dfsg-1_all
kmos_gen_telluric - Generate a TELLURIC frame
esorex kmos_gen_telluric [OPTIONS] FILE.sof
This recipe creates the TELLURIC frame needed by kmos_sci_red by merging the TELLURIC (produced by kmos_std_star), the static RESPONЅE frame and the TELLURIC_CORR (produced with molecfit). The way the frames are combined is controlled by the --method parameter: - 0 (default) : use TELLURIC and get zpoint from TELLURIC If TELLURIC missing, use RESPONSE and get zpoint from RESPONSE - 1 : use TELLURIC_CORR and get zpoint from TELLURIC_CORR - 2 : use RESPONSE and get zpoint from TELLURIC If TELLURIC missing, get zpoint from RESPONSE For missing ZPOINTs, use the average of other IFUs for the same detector. - 3 : use RESPONSE x TELLURIC_CORR and get zpoint from TELLURIC_CORR Input files: DO category Explanation Required ----------- ----------- -------- TELLURIC Produced by kmos_std_star N TELLURIC_CORR Produced by molecfit N RESPONSE static calibration N Output files: DO category Explanation ----------- ----------- TELLURIC_GEN Used by kmos_sci_red
--method <int> How the TELLURIC is generated (int; default: 0). The full name of this option for the EsoRex configuration file is kmos.kmos_gen_telluric.method [default = 0]. --b_samples <int> The number of samples in wavelength (int; default: -1). The full name of this option for the EsoRex configuration file is kmos.kmos_gen_telluric.b_samples [default = -1]. --fill_empty_ifus <bool> Flag to fill empty TELLURIC IFUs (only method 0) (bool; default: False). The full name of this option for the EsoRex configuration file is kmos.kmos_gen_telluric.fill_empty_ifus [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.
The full documentation for the kmos pipeline can be downloaded as a PDF file using the following URL: ftp://ftp.eso.org/pub/dfs/pipelines/kmos/kmos-pipeline-manual-2.9.pdf An overview over the existing ESO pipelines can be found on the web page https://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 https://packages.python.org/python-cpl/index.html for further information. The other recipes of the kmos pipeline are kmo_arithmetic(7), kmo_copy(7), kmo_fit_profile(7), kmo_fits_strip(7), kmo_make_image(7), kmo_noise_map(7), kmo_rotate(7), kmo_shift(7), kmo_sky_mask(7), kmo_stats(7), kmos_combine(7), kmos_dark(7), kmos_extract_spec(7), kmos_flat(7), kmos_gen_reflines(7), kmos_illumination(7), kmos_reconstruct(7), kmos_sci_red(7), kmos_sky_tweak(7), kmos_std_star(7), kmos_test(7), kmos_wave_cal(7)
Yves Jung <email@example.com>
Please report any problems to firstname.lastname@example.org. Alternatively, you may send a report to the ESO User Support Department <email@example.com>.
This file is part of the CRIRES Instrument Pipeline Copyright (C) 2002,2003 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., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA