FORS_PMOS_CALIB(7)
π FORS_PMOS_CALIB π (that's section 7 of the manuals, bestie)
okay so welcome to fors_pmos_calib, one of the fors recipes, and no cap this one is the β¨mask makerβ¨. sit down, grab a strawberry, we're doing this.
πΈ NAME πΈ
fors_pmos_calib β Determination of the extraction mask
β¨ SYNOPSIS β¨
esorex fors_pmos_calib [OPTIONS] FILE.sof
π¦ DESCRIPTION π¦
so this recipe is the one that goes and finds the reference lines on your PMOS arc lamp exposures, and then traces the spectral edges on the matching flat field exposures. all that detective work gets used to determine the spectral extraction mask that you then apply when you reduce your actual science data β which is done by the recipe fors_science. it's giving backstage crew, honestly. nobody claps for the mask, but nothing works without it.
this recipe accepts both FORS1 and FORS2 frames, icon behaviour. and heads up: the input arc lamps and flat field exposures are assumed to be obtained quasi-simultaneously, so that they'd be described by exactly the same instrument distortions. the vibe check is that they match, fr fr.
you must specify a line catalog, containing the wavelengths of the reference arc lamp lines used for the wavelength calibration. you may also specify a grism table (typically depending on the instrument mode, and in particular on the grism used): this table contains a default recipe parameter setting to control the way spectra are extracted for a specific instrument mode, as it is used for automatic run of the pipeline on Paranal and in Garching. if this table is specified, it will modify the default recipe parameter setting, with the exception of those parameters which have been explicitly modifyed on the command line. (yes, "modifyed". the manual said it, so we keep it π )
if a grism table is not specified, the input recipe parameter values will always be read from the command line, or from an esorex configuration file if present, or from their generic default values (that are rarely meaningful β lowkey tragic). and finally, a master bias frame must be input to this recipe. non-negotiable.
the products SPECTRA_DETECTION_PMOS, SLIT_MAP_PMOS, and DISP_RESIDUALS_PMOS, are just created if the --check parameter is set to true. so if you're like "where are my babies π", check --check.
the MASTER_DISTORTION_TABLE is marked as required, but it is not so if all slits have different offsets, and in the case of FORS1 observations made with the old TK2048EB4-1 1604 chip read in windowed mode (2048x400). okay so it's giving "required, but also not, depends" β iconic of it.
π₯ Input files
- DO category:
SCREEN_FLAT_PMOSβ Type:Rawβ Flat field exposures β Required: Y - DO category:
LAMP_PMOSβ Type:Rawβ Arc lamp exposure β Required: Y - DO category:
MASTER_BIASorBIASβ Type:Calibβ Bias frame β Required: Y - DO category:
MASTER_LINECATβ Type:Calibβ Line catalog β Required: Y - DO category:
GRISM_TABLEβ Type:Calibβ Grism table β Required:. - DO category:
MASTER_DISTORTION_TABLEβ Type:Calibβ Master distortions table β Required: Y
π€ Output files
- DO category:
MASTER_SCREEN_FLAT_PMOSβ Data type:FITS imageβ Combined (sum) flat field - DO category:
MASTER_NORM_FLAT_PMOSβ Data type:FITS imageβ Normalised flat field - DO category:
MAPPED_SCREEN_FLAT_PMOSβ Data type:FITS imageβ Wavelength calibrated flat field - DO category:
MAPPED_NORM_FLAT_PMOSβ Data type:FITS imageβ Wavelength calibrated normalised flat - DO category:
REDUCED_LAMP_PMOSβ Data type:FITS imageβ Wavelength calibrated arc spectrum - DO category:
DISP_COEFF_PMOSβ Data type:FITS tableβ Inverse dispersion coefficients - DO category:
DISP_RESIDUALS_PMOSβ Data type:FITS imageβ Residuals in wavelength calibration - DO category:
DISP_RESIDUALS_TABLE_PMOSβ Data type:FITS tableβ Residuals in wavelength calibration - DO category:
DELTA_IMAGE_PMOSβ Data type:FITS imageβ Offset vs linear wavelength calib - DO category:
WAVELENGTH_MAP_PMOSβ Data type:FITS imageβ Wavelength for each pixel on CCD - DO category:
SPECTRA_DETECTION_PMOSβ Data type:FITS imageβ Check for preliminary detection - DO category:
SLIT_MAP_PMOSβ Data type:FITS imageβ Map of central wavelength on CCD - DO category:
CURV_TRACES_PMOSβ Data type:FITS tableβ Spectral curvature traces - DO category:
CURV_COEFF_PMOSβ Data type:FITS tableβ Spectral curvature coefficients - DO category:
SPATIAL_MAP_PMOSβ Data type:FITS imageβ Spatial position along slit on CCD - DO category:
SPECTRAL_RESOLUTION_PMOSβ Data type:FITS tableβ Resolution at reference arc lines - DO category:
SLIT_LOCATION_PMOSβ Data type:FITS tableβ Slits on product frames and CCD
π OPTIONS π
okay bestie, here's the full roster. every single one, no skips. π
--dispersion<float> β Expected spectral dispersion (Angstrom/pixel) (float; default:0.0). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.dispersion[default =0.0].--peakdetection<float> β Initial peak detection threshold (ADU) (float; default:0.0). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.peakdetection[default =0.0].--wdegree<int> β Degree of wavelength calibration polynomial (int; default:0). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.wdegree[default =0].--wradius<int> β Search radius if iterating pattern-matching with first-guess method (int; default:4). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.wradius[default =4].--wreject<float> β Rejection threshold in dispersion relation fit (pixel) (float; default:0.7). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.wreject[default =0.7].--wcolumn<str> β Name of line catalog table column with wavelengths (str; default:WLEN). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.wcolumn[default =WLEN].--cdegree<int> β Degree of spectral curvature polynomial (int; default:0). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.cdegree[default =0].--cmode<int> β Interpolation mode of curvature solution (0= no interpolation,1= fill gaps,2= global model) (int; default:1). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.cmode[default =1].--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_pmos_calib.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_pmos_calib.endwavelength[default =0.0].--stack_method<str> β Frames combination method (str; default:average). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.stack_method[default =average].--minrejection<int> β Number of lowest values to be rejected (int; default:1). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.minrejection[default =1].--maxrejection<int> β Number of highest values to be rejected (int; default:1). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.maxrejection[default =1].--klow<float> β Low threshold in ksigma method (float; default:3.0). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.klow[default =3.0].--khigh<float> β High threshold in ksigma method (float; default:3.0). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.khigh[default =3.0].--kiter<int> β Max number of iterations in ksigma method (int; default:999). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.kiter[default =999].--ddegree<int> β Degree of flat field fitting polynomial along dispersion direction (int; default:-1). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.ddegree[default =-1].--dradius<int> β Smooth box radius for flat field along dispersion direction (int; default:10). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.dradius[default =10].--qc<bool> β Compute QC1 parameters (bool; default:True). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.qc[default =True].--check<bool> β Create intermediate products (bool; default:False). The full name of this option for the EsoRex configuration file isfors.fors_pmos_calib.check[default =False].
β¨ 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 SEE ALSO π
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_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_photometry(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 VERSION π
fors_pmos_calib 5.5.7
π AUTHOR π
Carlo Izzo <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>.
pt 2 is loadingβ¦ don't go anywhere bestie π«Ά
π LICENSE π
okay bestie, legal time, but make it cute πΈ
so this file is currently part of the FORS Instrument Pipeline, and the copyright belongs to:
Copyright (C) 2002-2010 European Southern Observatory
periodt. that's the whole vibe. π
π the part where they say "yes, you can have this" π
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.
so like β you can share it, you can remix it, you just gotta play by the GNU General Public License rules, the ones the Free Software Foundation wrote. version 2? slay. any later version? also slay, your call, bestie π
π the part where they're like "we promise nothing" π
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.
read it again for me bestie, because it matters: no warranty. not even the implied ones for MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. it hopes to be useful β that's the whole promise. the actual details live in the GNU General Public License, so go read those π«Ά
π¦ the "where's my copy" moment π¦
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
no license copy in your download? not a crisis, just write to the Free Software Foundation at:
Free Software Foundation, Inc.
51 Franklin St, Fifth Floor, Boston, MA 02110-1301 USA
iconic snail mail moment fr fr π
and that's the whole page, bestie β the last little line down there is just the footer doing its thing, telling you this page is fors_pmos_calib, version 5.5.7, living under FORS_PMOS_CALIB(7) with its date stamp. that's a wrap, go calibrate something gorgeous πβ¨π
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