VISIR_OLD_SPC_WCAL(7)
VISIR_OLD_SPC_WCAL π β¨
okay bestie, this is a visir recipe page β specifically the visir_old_spc_wcal one, from the visir recipes collection. buckle up π
πΈ NAME πΈ
visir_old_spc_wcal β the Old DRS detector's Spectroscopic wavelength calibration recipe. it does the wavelength thing. iconic behavior tbh π
β¨ SYNOPSIS β¨
esorex visir_old_spc_wcal [OPTIONS] FILE.sof
π¦ DESCRIPTION π¦
So this recipe estimates the dispersion relation using the atmospheric spectrum in a long-slit spectroscopy half-cycle frame. that's the whole job, and it eats it up, no crumbs π
The files listed in the Set Of Frames (sof-file) must be tagged like this β and yes, exactly like this, no improvising bestie:
VISIR-Long-Slit-Spectroscopy-file.fits SPEC_CAL_LMR_WCAL
VISIR-Quantum-Efficiency-Calibration-file.fits SPEC_CAL_QEFF
VISIR-Atmospheric-Emission-Lines-Calibration-file.fits SPEC_CAL_LINES
And additionally (bonus round π«Ά), a bad pixel map with a PRO.CATG of SPEC_BPM may be added to the Set Of Frames with tag: BPM.
π OPTIONS π
--auto_bpm <bool>β automatic detection and correction of bad pixels. it's abool, default:True. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.auto_bpm [default = True]. β¨--plot <int>β the recipe can produce a number of predefined plots. Zero means none of the plots are produced, while increasing values (e.g.1or2) increases the number of plots produced. If the plotting fails, a warning is produced, and the recipe continues β she's resilient, she moves on π
The default behaviour of the plotting is to use gnuplot (with option -persist). The recipe currently produces 1D-plots using gnuplot commands.
The recipe user can control the actual plotting-command used by the recipe to create the plot by setting the environment variable CPL_PLOTTER. Currently, if CPL_PLOTTER is set it must contain the string Β΄gnuplotΒ΄. Setting it to Β΄cat > my_gnuplot_$$.txtΒ΄ causes a number of ASCII-files to be created, which each produce a plot when given as standard input to gnuplot (e.g. later or on a different computer). A finer control of the plotting options can be obtained by writing an executable script, e.g. my_gnuplot.pl, that executes gnuplot after setting the desired gnuplot options (e.g. set terminal pslatex color) and then setting CPL_PLOTTER to my_gnuplot.pl.
The predefined plots include plotting of images. Images can be plotted not only with gnuplot, but also using the pnm format. This is controlled with the environment variable CPL_IMAGER. If CPL_IMAGER is set to a string that does not contain the word gnuplot, the recipe will generate the plot in pnm format. E.g. setting CPL_IMAGER to Β΄display - &Β΄ will produce a gray-scale image using the image viewer display. It's an int, default: 0. The full name of this option for the EsoRex configuration file is visir.visir_old_spc_wcal.plot [default = 0]. π
--slit_skew <float>β Distortion correction: Skew of slit (degrees) (clockwise). it's afloat, default:0.52. The full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.phi [default = 0.52]. π¦--spectrum_skew <float>β Distortion correction: LMR Skew of spectrum (degrees) (counter-clockwise). Not used in High Resolution. it's afloat, default:1.73. The full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.ksi [default = 1.73]. β--vert_arc <float>β Distortion correction: LR Detector vertical curvature (pixel). Reduced by a factor4in MR. Not used in HR A-side. Increased by a factor115/52in HR B-side. it's afloat, default:-0.8. The full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.eps [default = -0.8]. πΈ--hori_arc <float>β Distortion correction: LMR Detector horizontal curvature (pixel). Increased by a factor1.5in HR A-side. Reduced by a factor2in HR B-side. it's afloat, default:0.0. The full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.delta [default = 0.0]. π--rl <int>β Reject leftmost columns in spectrum extraction, zero means all columns on the left are used. In cross-dispersion mode a (small) negative number may be used (pixel). it's anint, default:0. The full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.reject_left [default = 0]. π--rr <int>β Reject rightmost columns in spectrum extraction, zero means all columns on the right are used. In cross-dispersion mode a (small) negative number may be used (pixel). it's anint, default:0. The full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal.reject_right [default = 0]. π
ngl bestie, 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. π
π₯ SEE ALSO π₯
The full documentation for the visir pipeline can be downloaded as a PDF file using the following URL:
ftp://ftp.eso.org/pub/dfs/pipelines/visir/visir-pipeline-manual-1.4.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 visir pipeline are β and she listed ALL of them, no cap π:
visir_img_dark(7)visir_img_ff(7)visir_img_reduce(7)visir_img_trans(7)visir_old_img_combine(7)visir_old_img_phot(7)visir_old_spc_obs(7)visir_old_spc_obs_ech(7)visir_old_spc_phot(7)visir_old_spc_phot_ech(7)visir_old_spc_wcal_ech(7)visir_old_util_destripe(7)visir_spc_reduce(7)visir_util_apply_calib(7)visir_util_clip(7)visir_util_convert_weight(7)visir_util_detect_shift(7)visir_util_img_std_cat(7)visir_util_join(7)visir_util_qc(7)visir_util_repack(7)visir_util_run_swarp(7)visir_util_spc_std_cat(7)visir_util_spc_txt2fits(7)visir_util_undistort(7)
π VERSION π
visir_old_spc_wcal 4.4.2 β that's the one, periodt π
π§ AUTHOR π§
Lars Lundin <https://support.eso.org> β thank you king π«Ά
π BUG REPORTS π
Please report any problems to https://support.eso.org. Alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>. they wanna hear from u fr fr, don't be shy π
π LICENSE π
This file is part of the VISIR Instrument Pipeline Copyright (C) 2004, 2005 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
and that's the whole page bestie π this was visir_old_spc_wcal, version 4.4.2, from the VISIR_OLD_SPC_WCAL(7) manual, dated 4.4.2 β slay, go calibrate those wavelengths, iykyk ππ¦β¨
π¦ where this page comes from
- debian bookworm: cpl-plugin-visir-doc 4.4.2+dfsg-1 Β· GPL-v2+
- ubuntu noble: cpl-plugin-visir-doc 4.4.2+dfsg-1 Β· GPL-v2+
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms