FORS_ALIGN_SKY_LSS(7)

πŸ“¦ version 5.5.7, in ubuntu jammy, ubuntu noble

🌈 FORS_ALIGN_SKY_LSS ✨

okay bestie, gather round, because this is the fors_align_sky_lss manual page from the fors recipes, and she is lowkey a baddie πŸ’…


πŸ¦‹ 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.


✨ SYNOPSIS

esorex fors_align_sky_lss [OPTIONS] FILE.sof

πŸ’– DESCRIPTION

so here's the tea πŸ“: 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 πŸ‘‘

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 ✨

πŸ“₯ Input files:

  • SCIENCE_UNBIAS_MXU or SCIENCE_UNFLAT_MXU or STANDARD_UNBIAS_MXU or STANDARD_UNFLAT_MXU β€” Type: Calib β€” Frame with sky lines β€” Required: Y
  • DISP_COEFF_MXU β€” Type: Calib β€” Dispersion solution β€” Required: Y
  • SLIT_LOCATION_MXU β€” Type: Calib β€” Slit location on CCD β€” Required: Y
  • MASTER_SKYLINECAT β€” Type: Calib β€” Catalog of sky lines β€” Required: .
  • GRISM_TABLE β€” Type: Calib β€” Grism table β€” Required: .

πŸ“€ Output files:

  • SKY_SHIFTS_LONG_SCI_MXU β€” Data type: FITS table β€” Observed sky lines offsets
  • WAVELENGTH_MAP_SCI_MXU β€” Data type: FITS image β€” Wavelength mapped on CCD
  • DISP_COEFF_SCI_MXU β€” Data type: FITS image β€” Upgraded dispersion solution

πŸŽ€ OPTIONS

one bullet per option, no skipping, we respect the whole menu πŸ’œ

  • --dispersion <float> β€” Expected spectral dispersion, in Angstrom/pixel (float; default: 0.0). The full name of this option for the EsoRex configuration file is fors.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 is fors.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 is fors.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 is fors.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 is fors.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. 🫢

πŸ”₯ 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) πŸ’«


πŸ‘‘ VERSION

fors_align_sky_lss 5.5.7


🌸 AUTHOR

Carlo Izzo <usd-help@eso.org>


πŸ’€ 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 πŸ™ˆ


πŸ“œ 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 🧚

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 πŸ’…βœ¨

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