XSH_WAVECAL(7)
β¨ XSH_WAVECAL β¨
okay bestie, welcome to xsh_wavecal, a recipe from the xshoo pipeline (that's the manual family it lives in, XSH_WAVECAL(7)). this one's whole job? detecting and following arc lines in a fully illuminated slit frame, then figuring out the arclines tilt and the instrument resolution. it's giving detective energy but for photons. π
πΈ NAME πΈ
xsh_wavecal β compute arclines tilt and instrument resolution. yes ma'am, that's the whole vibe. π
π¦ SYNOPSIS π¦
esorex xsh_wavecal [OPTIONS] FILE.sof
π DESCRIPTION π
so this recipe detects and follows arc lines in a fully illuminated slit frame. that's it, that's the mission. π₯
π§ Input Frames (the guest list, no plus-ones unless marked)
- Raw frame (Tag =
ARC_SLIT_arm) - Arc Line List (Tag =
ARC_LINE_LIST_arm) - Master Bias (Tag =
MASTER_BIAS_arm) - [OPTIONAL] Master Dark (Tag =
MASTER_DARK_arm) - Order Table (Tag =
ORDER_TABLE_EDGES_arm) - [poly mode] Wave Solution (Tag =
WAVE_TAB_2D_arm) - [poly mode] Theoretical Map (Tag =
THEO_TAB_spec_arm, spec=SING/IFU) - [physical model mode] Model cfg tab (Tag =
XSH_MOD_CFG_TAB_arm)- [OPTIONAL] A non-linear badpixel map (Tag =
BP_MAP_NL_arm) - [OPTIONAL] A reference badpixel map (Tag =
BP_MAP_RP_arm)
- [OPTIONAL] A non-linear badpixel map (Tag =
- [OPTIONAL-To compute spectral resolution] Dispersion Table Frame (Tag =
DISP_TAB_arm)
Prepare PRE structures. (yes that's literally what it says, bestie β prepare them. π«)
then the glow-up sequence:
- Subtract the master Dark (UVB, VIS and NIR)
- Substract the master Bias (UVB and VIS)
- Divide by Flat.
then:
- Detect and follow arc lines. π
π Products (the receipts)
- Wavelength solution, PRO.CATG =
WAVE_TAB_ARC_SLIT_arm[if poly mode] - Linetilt list, PRO.CATG =
TILT_TAB_SLIT_arm - Residuals table, PRO.CATG =
RESID_TAB_GOOD_LINES_arm - Wave Map, PRO.CATG =
WAVE_MAP_arm[if model-wavemap-compute=TRUE] - In case of IFU mode cdata previous producs repat for each IFU slices
- Arc frame, Bias subtracted in PRE format, PRO.CATG =
ARC_BIAS_SUBTRACT_arm - If arm=UVB/VIS and PRO.CATG=
ARC_NIR_ONif arm=NIR - Arc frame, Bias subtracted, FLAT-FIELDED, PRO.CATG =
WAVECAL_FLATFIELDED_arm
π OPTIONS π
every single one, bestie. i'm not skipping a single flag, that's not the energy we bring. π«Ά
--keep-temp <str>β if it'sΒ΄noΒ΄, temporary files get deleted. (str; default:Β΄noΒ΄). the full name of this option for the EsoRex configuration file isxsh.xsh_wavecal.keep-temp[default = no].--debug-level <str>β extra xshooter debug level, pick fromΒ΄noneΒ΄,Β΄lowΒ΄,Β΄mediumΒ΄,Β΄highΒ΄. (str; default:Β΄noneΒ΄). full name for EsoRex config:xsh.xsh_wavecal.debug-level[default = none].--time-stamp <bool>β slap a timestamp onto the product file name, cute. (bool; default: False). full name for EsoRex config:xsh.xsh_wavecal.time-stamp[default = False].--decode-bp <int>β integer representation of the bits to be considered bad when decoding the bad pixel mask pixel values. the most frequent codes relevant for the user, memorise these fr fr:0: good pixel,8: pick-up noise,16: cosmic-ray removed,32: cosmic-ray unremoved,128: calibration file defect,256: hot pixel,512: dark pixel,4096: A/D converted saturation,32768: non linear pixel,1048576: extrapolated flux in NIR,4194304: Interpolated flux during extraction. (int; default: 2144337919). full name for EsoRex config:xsh.xsh_wavecal.decode-bp[default = 2144337919].--pre-overscan-corr <int>β pre-overscan correction.0: no correction,1: mean overscan correction,2: mean prescan correction,3: (mean pre+mean overscan)/2 correction. (int; default: 1). full name for EsoRex config:xsh.xsh_wavecal.pre-overscan-corr[default = 1].--followarclines-search-window-half-size <int>β half window size (HWS) in pixels (Y axis) of the search window for each line. (int; default: 13). full name for EsoRex config:xsh.xsh_wavecal.followarclines-search-window-half-size[default = 13].--followarclines-order-edges-mask <int>β nb of pixels suppressed (X) from edges of search window. (int; default: 3). full name for EsoRex config:xsh.xsh_wavecal.followarclines-order-edges-mask[default = 3].--followarclines-min-sn <float>β minimum Signal over Noise ratio at center to keep the line (6for IFU,15for SLIT). (float; default: -1.0). full name for EsoRex config:xsh.xsh_wavecal.followarclines-min-sn[default = -1.0].--tilt-clip-kappa <float>β multiple of sigma in sigma clipping for evaluating tilt. (float; default: 2.5). full name for EsoRex config:xsh.xsh_wavecal.tilt-clip-kappa[default = 2.5].--tilt-clip-niter <int>β number of iterations in sigma clipping for evaluating tilt. (int; default: 5). full name for EsoRex config:xsh.xsh_wavecal.tilt-clip-niter[default = 5].--tilt-clip-frac <float>β minimal fraction of points accepted / total in sigma clipping for evaluating tilt. (float; default: 0.7). full name for EsoRex config:xsh.xsh_wavecal.tilt-clip-frac[default = 0.7].--specres-clip-kappa <float>β multiple of sigma in sigma clipping for evaluating spectral resolution. (float; default: 2.5). full name for EsoRex config:xsh.xsh_wavecal.specres-clip-kappa[default = 2.5].--specres-clip-niter <int>β number of iterations in sigma clipping for evaluating spectral resolution. (int; default: 5). full name for EsoRex config:xsh.xsh_wavecal.specres-clip-niter[default = 5].--specres-clip-frac <float>β minimal fraction of points accepted / total in sigma clipping for evaluating spectral resolution. (float; default: 0.7). full name for EsoRex config:xsh.xsh_wavecal.specres-clip-frac[default = 0.7].
heads up bestie: you can totally make a configuration file holding all these options plus suitable default values. the details are in the 'esorex --help' command. go read it, i'll wait. π
π SEE ALSO π
the full documentation for the xshoo pipeline can be downloaded as a PDF file using this URL:
ftp://ftp.eso.org/pub/dfs/pipelines/xshoo/xshoo-pipeline-manual-12.1.pdf
an overview over the existing ESO pipelines lives on this web page: https://www.eso.org/sci/software/pipelines/.
basic documentation about the EsoRex program is in 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.
the other recipes of the xshoo pipeline, aka the whole friend group, are: xsh_2dmap(7), xsh_cfg_recover(7), xsh_flexcomp(7), xsh_geom_ifu(7), xsh_lingain(7), xsh_mbias(7), xsh_mdark(7), xsh_mflat(7), xsh_orderpos(7), xsh_predict(7), xsh_respon_slit_nod(7), xsh_respon_slit_offset(7), xsh_respon_slit_stare(7), xsh_scired_ifu_offset(7), xsh_scired_ifu_offset_drl(7), xsh_scired_ifu_stare(7), xsh_scired_ifu_stare_drl(7), xsh_scired_slit_nod(7), xsh_scired_slit_offset(7), xsh_scired_slit_stare(7), xsh_util_physmod(7).
β VERSION β
xsh_wavecal 3.5.3
π AUTHOR π
L.Guglielmi <amodigli@eso.org> β shoutout to the icon who made this. π
π¦ BUG REPORTS π¦
please report any problems to amodigli@eso.org. alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>. if something's cursed, tell them, not me. π
π LICENSE π
this file is part of the X-shooter Instrument Pipeline Copyright (C) 2006 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., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA.
and that's the whole page, bestie!! π«Ά this was xsh_wavecal version 3.5.3, served fresh from the xshoo recipes, dated 3.5.3, filed under XSH_WAVECAL(7). now go calibrate something and slay. πβ¨π
π¦ where this page comes from
- ubuntu jammy: cpl-plugin-xshoo-doc 3.5.3+dfsg-1build1 Β· GPL-v2+
- ubuntu noble: cpl-plugin-xshoo-doc 3.5.3+dfsg-1build4 Β· GPL-v2+
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms