FORS_ALIGN_SKY_LSS(7)
π FORS_ALIGN_SKY_LSS β¨
okay bestie, gather round, because this is the fors_align_sky_lss manual page from the fors recipes, and she is lowkey a baddie π
π¦ NAME
fors_align_sky_lss β upgrade wavelength solution using sky lines. yes that's the whole vibe, she takes your wavelength solution and makes it better, no cap.
β¨ SYNOPSIS
esorex fors_align_sky_lss [OPTIONS] FILE.sof
π DESCRIPTION
so here's the tea π: this recipe aligns the wavelength solution β the one based on your arc lamp exposure β using a whole set of sky lines that got observed on a scientific exposure. it's giving glow-up, but for wavelengths.
The input scientific frames are the ones produced by the recipes fors_remove_bias and fors_flatfield. You can specify an input catalog of sky lines if you want, or an internal one gets used instead. your call, queen π
This recipe should be applied to LSS or long-slit-like data (that means MOS/MXU with all slits at the same offset, iykyk). For multi-slit MOS/MXU data, use recipe fors_align_sky instead β she's the one built for that job. Please refer to the FORS PIpeline UserΒ΄s Manual for more details.
In the table below, the MXU acronym can alternatively be read as MOS and LSS, and SCI as STD. cute, right? interchangeable β¨
π₯ Input files:
SCIENCE_UNBIAS_MXUorSCIENCE_UNFLAT_MXUorSTANDARD_UNBIAS_MXUorSTANDARD_UNFLAT_MXUβ Type: Calib β Frame with sky lines β Required: YDISP_COEFF_MXUβ Type: Calib β Dispersion solution β Required: YSLIT_LOCATION_MXUβ Type: Calib β Slit location on CCD β Required: YMASTER_SKYLINECATβ Type: Calib β Catalog of sky lines β Required:.GRISM_TABLEβ Type: Calib β Grism table β Required:.
π€ Output files:
SKY_SHIFTS_LONG_SCI_MXUβ Data type: FITS table β Observed sky lines offsetsWAVELENGTH_MAP_SCI_MXUβ Data type: FITS image β Wavelength mapped on CCDDISP_COEFF_SCI_MXUβ Data type: FITS image β Upgraded dispersion solution
π OPTIONS
one bullet per option, no skipping, we respect the whole menu π
--dispersion<float> β Expected spectral dispersion, in Angstrom/pixel (float; default:0.0). The full name of this option for the EsoRex configuration file isfors.fors_align_sky_lss.dispersion[default =0.0].--startwavelength<float> β Start wavelength in spectral extraction (float; default:0.0). The full name of this option for the EsoRex configuration file isfors.fors_align_sky_lss.startwavelength[default =0.0].--endwavelength<float> β End wavelength in spectral extraction (float; default:0.0). The full name of this option for the EsoRex configuration file isfors.fors_align_sky_lss.endwavelength[default =0.0].--skyalign<int> β Polynomial order for sky lines alignment (int; default:0). The full name of this option for the EsoRex configuration file isfors.fors_align_sky_lss.skyalign[default =0].--wcolumn<str> β Name of sky line catalog table column with wavelengths (str; default:WLEN). The full name of this option for the EsoRex configuration file isfors.fors_align_sky_lss.wcolumn[default =WLEN].
ngl, it's also 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«Ά
π₯ 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-4.9.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 fors pipeline are fors_align_sky(7), fors_bias(7), fors_calib(7), fors_config(7), fors_dark(7), fors_detect_objects(7), fors_detect_spectra(7), fors_extract(7), fors_extract_objects(7), fors_extract_slits(7), fors_flatfield(7), fors_img_science(7), fors_img_screen_flat(7), fors_img_sky_flat(7), fors_normalise_flat(7), fors_photometry(7), fors_pmos_calib(7), fors_pmos_extract(7), fors_pmos_science(7), fors_remove_bias(7), fors_resample(7), fors_science(7), fors_spec_mflat(7), fors_subtract_sky(7), fors_subtract_sky_lss(7), fors_sumflux(7), fors_trace_flat(7), fors_wave_calib(7), fors_wave_calib_lss(7), fors_zeropoint(7) π«
π VERSION
fors_align_sky_lss 5.5.7
πΈ AUTHOR
Carlo Izzo <usd-help@eso.org>
π 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>. they're nice, they don't bite, fr fr π
π 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
okay that's the whole page bestie, every single flag, every file, every URL, nothing skipped π§
signing off: this was fors_align_sky_lss version 5.5.7, dated 5.5.7, from the fors recipes manual, page FORS_ALIGN_SKY_LSS(7) β stan behavior, go forth and align π
β¨
π¦ where this page comes from
- ubuntu jammy: cpl-plugin-fors-doc 5.5.7+dfsg-2build1 Β· GPL-v2+
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