FORS_PHOTOMETRY(7)
β¨ FORS_PHOTOMETRY β¨
okay bestie, sit down, we're doing fors_photometry β it's a recipe from the fors pipeline family and it lives in section 7 of the manual. What does it do? It computes the corrected flatfield. That's it, that's the whole gig. π
πΈ SYNOPSIS πΈ
esorex fors_photometry [OPTIONS] FILE.sof
π¦ DESCRIPTION π¦
π Input files (what you gotta feed it)
Each one has a DO category, a type, an explanation, and a number. No skipping, okay?
PHOT_TABLEβ FITS table β expected extinction params β number:1ALIGNED_PHOTβ FITS table β photometry β number:1+MASTER_SKY_FLAT_IMGβ FITS image β master flat field β number:1
β¨ Output files (what it hands back to you)
PHOT_COEFF_TABLEβ FITS image β observed extinction coefficientsCORRECTION_MAPβ FITS image β correction map (magnitude)CORRECTION_FACTORβ FITS image β correction map (flux)MASTER_FLAT_IMGβ FITS image β corrected master flat field
likeβ¦ the glow-up of flatfields. periodt. π
π OPTIONS π
Every single one, in order, no crumbs left behind. Each one also has a full name for the EsoRex configuration file, because of course it does.
--fitz<bool> β fit zeropoint (bool; default:True). The full name of this option for the EsoRex configuration file isfors.fors_photometry.fitz[default = True].--fit_all_mag<bool> β always fit star magnitudes (bool; default:False). The full name of this option for the EsoRex configuration file isfors.fors_photometry.fit_all_mag[default = False].--fite<str> β fit atmospheric extinctions (str; default:pernight). The full name of this option for the EsoRex configuration file isfors.fors_photometry.fite[default = pernight].--fitc<bool> β fit color correction term (bool; default:False). The full name of this option for the EsoRex configuration file isfors.fors_photometry.fitc[default = False].--use_all_stars<bool> β use also non-standard stars to fit polynomial f (bool; default:False). The full name of this option for the EsoRex configuration file isfors.fors_photometry.use_all_stars[default = False].--degreef1<int> β flatfield correction map polynomial degree (x) (int; default:0). The full name of this option for the EsoRex configuration file isfors.fors_photometry.degreef1[default = 0].--degreef2<int> β flatfield correction map polynomial degree (y), or negative for triangular coefficient matrix (int; default:-1). The full name of this option for the EsoRex configuration file isfors.fors_photometry.degreef2[default = -1].--degreep<int> β extinction/color coupling degree (int; default:0). The full name of this option for the EsoRex configuration file isfors.fors_photometry.degreep[default = 0].--mjd_obs_target<float> β MJD-OBS used to match the raw frame from whichEXTINCTION_PER_NIGHTandPHOT_COEFFinherit MJD-OBS. If negative, the MJD-OBS of the first raw frame is used (float; default:-1.0). The full name of this option for the EsoRex configuration file isfors.fors_photometry.mjd_obs_target[default = -1.0].
π‘ heads up bestie: you can make a configuration file holding these options, along with suitable default values. Please refer to the details provided by the esorex --help command.
π SEE ALSO π
The full documentation for the fors pipeline can be downloaded as a PDF file using this 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.
You can also call the pipelines from python using the python-cpl package. See:
https://packages.python.org/python-cpl/index.html
for further information.
And now, the whole friend group β the other recipes of the fors pipeline, all linked up:
fors_align_sky(7), fors_align_sky_lss(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_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)
β VERSION β
fors_photometry 5.5.7
π AUTHOR π
Jonas M. Larsen <usd-help@eso.org>
π BUG REPORTS π
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>.
(not me telling you to actually email them, they're lovely, they want the bug reports fr fr π«Ά)
π LICENSE π
This file is currently part of the FORS Instrument Pipeline Copyright (C) 2002-2011 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
and that's the whole page, bestie β fors_photometry version 5.5.7, chillin' on the FORS_PHOTOMETRY(7) page. go correct those flats, you absolute icon πβ¨
π¦ where this page comes from
- ubuntu jammy: cpl-plugin-fors-doc 5.5.7+dfsg-2build1 Β· GPL-v2+
- ubuntu noble: cpl-plugin-fors-doc 5.5.7+dfsg-2build1 Β· GPL-v2+
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms