VISIR_OLD_SPC_WCAL_ECH(7)
π VISIR_OLD_SPC_WCAL_ECH π
okay bestie, welcome to section 7 of the manuals β the visir recipes corner of the universe β where we meet visir_old_spc_wcal_ech, aka the Old DRS detector's Spectroscopic wavelength calibration recipe in Echelle mode. she's giving very niche, very powerful, very wavelength. let's get into it β¨
π SYNOPSIS π
esorex visir_old_spc_wcal_ech [OPTIONS] FILE.sof
that's it, that's the summoning ritual π
πΈ DESCRIPTION πΈ
so what does she actually do? this recipe estimates the dispersion relation using the atmospheric spectrum in a grism spectroscopy half-cycle frame. atmospheric lines are literally her best friend, no cap π
the files listed in the Set Of Frames (sof-file) must be tagged like this:
VISIR-Echelle-Spectroscopy-file.fits SPEC_CAL_HRG_WCAL
VISIR-Quantum-Efficiency-Calibration-file.fits SPEC_CAL_QEFF
VISIR-Atmospheric-Emission-Lines-Calibration-file.fits SPEC_CAL_LINES
and bonus round: a bad pixel map with a PRO.CATG of SPEC_BPM may be added to the Set Of Frames with the tag BPM. optional but she'll happily accept it π«Ά
β¨ OPTIONS β¨
--auto_bpm<bool> β automatic detection and correction of bad pixels. it's a bool, and the default isTrue. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.auto_bpm[default = True]. she's automatic, she's correcting, she's that girl π--plot<int> β okay this one is a whole saga, sit down π. the recipe can produce a number of predefined plots. zero means none of the plots are produced, while increasing values (e.g.1or2) increase the number of plots produced. if the plotting fails a warning is produced, and the recipe continues (she does not crash out, she's resilient). the default behaviour of the plotting is to usegnuplot(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 variableCPL_PLOTTER. currently, ifCPL_PLOTTERis 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 settingCPL_PLOTTERtomy_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 variableCPL_IMAGER. ifCPL_IMAGERis set to a string that does not contain the word gnuplot, the recipe will generate the plot in pnm format. e.g. settingCPL_IMAGERto 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 isvisir.visir_old_spc_wcal_ech.plot[default = 0]. obsessed with the flexibility honestly π--slit_skew<float> β distortion correction: skew of slit (degrees) (clockwise). it's a float; default:0.0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.phi[default = 0.0]. yes the option name and the config name are different, that's just her vibe π--spectrum_skew<float> β distortion correction: LMR skew of spectrum (degrees) (counter-clockwise). not used in High Resolution. float; default:0.0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.ksi[default = 0.0].--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. float; default:0.0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.eps[default = 0.0]. math is math bestie π₯--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. float; default:0.0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.delta[default = 0.0].--orderoffset<int> β Echelle order offset. the offset is relative to the main order. the allowed range of offsets depend on the selected grism. the offset can never exceed +/-4. if the main order is e.g.8an order offset of+1will cause the recipe to base the data reduction on order9. with a positive order offset the central wavelength becomes smaller, while for a negative order offset the central wavelength becomes larger. int; default:0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.orderoffset[default = 0]. shifting orders like a main character 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). int; default:0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.reject_left[default = 0].--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). int; default:0. the full name of this option for the EsoRex configuration file isvisir.visir_old_spc_wcal_ech.reject_right[default = 0].
ngl, 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 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(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). the whole friend group, fr fr π«Ά
π« VERSION π«
visir_old_spc_wcal_ech 4.4.2
π AUTHOR π
Lars Lundin <https://support.eso.org> β icon behavior, honestly β
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>. (not me telling you to file your bugs, but like, do it 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_ech, version 4.4.2, living her best life in the VISIR_OLD_SPC_WCAL_ECH(7) manual β wavelength calibration in Echelle, atmospheric spectrum edition. slay, calibrate, periodt β¨π
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