XSH_RESPON_SLIT_STARE(7)

πŸ“¦ version 3.5.3, in ubuntu jammy, ubuntu noble

XSH_RESPON_SLIT_STARE πŸ’–

ok so bestie, this is the manual page for xsh_respon_slit_stare β€” section 7 of the xshoo recipes manual. grab a snack, we're doing science. πŸŽ€


✨ NAME ✨

xsh_respon_slit_stare β€” compute the response function in SLIT stare mode. yes that's the whole name. iconic of it honestly. πŸ’…


✨ SYNOPSIS ✨

esorex xsh_respon_slit_stare [OPTIONS] FILE.sof

✨ DESCRIPTION ✨

so this recipe computes the response function for whichever arm you hand it. no cap. πŸ¦‹

Here's the whole Input Frames situation for the arm β€” read it like a checklist bestie, because it kinda is one:

  • A RAW frame (Tag = STD_FLUX_SLIT_STARE_arm, Type = RAW)
  • [UVB,VIS] A master bias frame (Tag = MASTER_BIAS_arm, Type = PRE)
  • A master dark frame (Tag = MASTER_DARK_arm Type = PRE)
  • A master flat frame (Tag = MASTER_FLAT_SLIT_arm Type = PRE)
  • An order table frame (Tag = ORDER_TAB_EDGES_arm Type = ORD)
  • A wave solution frame (Tag = WAVE_TAB_2D_arm, Type = WAV)
  • [OPTIONAL] Table with dispersion coefficients (Tag = DISP_TAB_arm)
  • [OPTIONAL] A telluric model catalog (Tag = TELL_MOD_CAT_arm arm=VIS,NIR)
  • A standard star fluxes catalog (Tag = FLUX_STD_CATALOG_arm Type = FLX)
  • A table to set response sampling points (Tag = RESP_FIT_POINTS_CAT_arm)
  • An atmospheric extinction table (Tag = ATMOS_EXT_arm)
    • if provided this is the one used to flux calibrate the spectra ✨
  • [OPTIONAL,physmod mode] A table listing sky line positions (Tag = SKY_LINE_LIST_arm)
    • this is used to be able to control quality of sky subtraction, for example projecting guess positions on the product SCI_SLIT_STARE_SUB_SKY_arm
    • and it is required if sky-method=BSPLINE πŸ‘€

Products :

  • [If STD is in catal] The response ord-by-ord function (Tag = PREFIX_RESPONSE_ORDER1D_SLIT_arm)
  • [If STD is in catal] The response merged function (Tag = PREFIX_RESPONSE_MERGE1D_SLIT_arm)
  • The extracted 2D specturm (Tag = PREFIX_ORDER2D_arm)
  • The extracted 1D specturm (Tag = PREFIX_ORDER1D_arm)
  • The merged 2D specturm (Tag = PREFIX_MERGE2D_arm)
  • The merged 1D specturm (Tag = PREFIX_MERGE1D_arm)
  • The merged 2D sky frame (Tag = SLY_SLIT_MERGED2D)
  • [If STD is in catal] Flux calibrated merged 2D spectrum (Tag = PREFIX_FLUX_ORDER2D_arm)
  • [If STD is in catal] Flux calibrated merged 1D spectrum (Tag = PREFIX_FLUX_ORDER1D_arm)
  • [If STD is in catal] Flux calibrated merged 2D spectrum (Tag = PREFIX_FLUX_MERGE2D_arm)
  • [If STD is in catal] Flux calibrated merged 1D spectrum (Tag = PREFIX_FLUX_MERGE1D_arm)
  • [If STD is in catal] The efficiency (Tag = EFFICIENCY_SLIT_arm)
  • where PREFIX is SCI, FLUX, TELL if input raw DPR.TYPE contains OBJECT or FLUX or TELLURIC
and yes, "specturm" is spelled like that in the original and I refuse to gaslight you about it 😭 we keep the typos, that's the rule fr fr

✨ OPTIONS ✨

every single one, bestie, in order, no skips 🫢

  • --keep-temp <str> β€” If Β΄noΒ΄, temporary files are deleted. (str; default: Β΄noΒ΄). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.keep-temp [default = no].
  • --debug-level <str> β€” Additional xshooter debug level. One of Β΄noneΒ΄, Β΄lowΒ΄, Β΄mediumΒ΄, Β΄highΒ΄ (str; default: Β΄noneΒ΄). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.debug-level [default = none].
  • --time-stamp <bool> β€” Add timestamp to product file name. (bool; default: False). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.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. Most frequent codes relevant for the user: 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). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.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). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.pre-overscan-corr [default = 1].
  • --background-edges-margin <int> β€” X margin to order edge to define background sampling points (int; default: 1). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.background-edges-margin [default = 1].
  • --background-poly-deg-y <int> β€” Poly mode fit deg along Y. (int; default: 9). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.background-poly-deg-y [default = 9].
  • --background-poly-deg-x <int> β€” Poly mode fit deg along X. (int; default: 9). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.background-poly-deg-x [default = 9].
  • --background-poly-kappa <float> β€” Poly mode kappa value of kappa-sigma-clip outliers removal. (float; default: 10.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.background-poly-kappa [default = 10.0].
  • --removecrhsingle-sigmalim <float> β€” Poisson fluctuation threshold to flag CRHs (see van Dokkum, PASP,113,2001,p1420-27) (float; default: 20.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.removecrhsingle-sigmalim [default = 20.0].
  • --removecrhsingle-flim <float> β€” Minimum contrast between the Laplacian image and the fine structure image that a point must have to be flagged as CRH. (see van Dokkum, PASP,113,2001,p1420-27) (float; default: 2.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.removecrhsingle-flim [default = 2.0].
  • --removecrhsingle-niter <int> β€” Max number of iterations (int; default: 4). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.removecrhsingle-niter [default = 4].
  • --rectify-kernel <str> β€” Name of the Interpolation Kernel Used. Possible values are: tanh, sinc, sinc2, lanczos, hamming, hann. (str; default: Β΄tanhΒ΄). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.rectify-kernel [default = tanh].
  • --rectify-radius <float> β€” Rectify Interpolation radius [bin units]. (float; default: 2.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.rectify-radius [default = 2.0].
  • --rectify-bin-lambda <float> β€” Wavelength step in the output spectrum [nm] (float; default: -1.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.rectify-bin-lambda [default = -1.0].
  • --rectify-bin-slit <float> β€” Spatial step along the slit in the output spectrum [arcsec] (float; default: -1.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.rectify-bin-slit [default = -1.0].
  • --localize-method <str> β€” Localization method (MANUAL, MAXIMUM, GAUSSIAN) used to detect the object centroid and height on the slit (str; default: Β΄MANUALΒ΄). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-method [default = MANUAL].
  • --localize-chunk-nb <int> β€” Number of chunks in the full spectrum to localize the object (int; default: 10). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-chunk-nb [default = 10].
  • --localize-thresh <float> β€” Threshold relative to the peak intensity below which the edges of the object are detected for MAXIMUM localization (float; default: 0.1). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-thresh [default = 0.1].
  • --localize-deg-lambda <int> β€” Degree in lambda in the localization polynomial expression slit=f(lambda), used only for MAXIMUM and GAUSSIAN (int; default: 0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-deg-lambda [default = 0].
  • --localize-slit-position <float> β€” Object position on the slit for MANUAL localization [arcsec] (float; default: 0.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-slit-position [default = 0.0].
  • --localize-slit-hheight <float> β€” Object half height on the slit for MANUAL localization [arcsec] (float; default: 2.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-slit-hheight [default = 2.0].
  • --localize-kappa <float> β€” Kappa value for sigma clipping in the localization polynomial fit (float; default: 3.0). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-kappa [default = 3.0].
  • --localize-niter <int> β€” Number of iterations for sigma clipping in the localization polynomial fit (int; default: 3). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-niter [default = 3].
  • --localize-use-skymask <bool> β€” TRUE if we want to mask sky lines using SKY_LINE_LIST file. (bool; default: False). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.localize-use-skymask [default = False].
  • --sky-subtract <bool> β€” TRUE to use subtract sky single. (bool; default: True). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.sky-subtract [default = True].
  • --sky-bspline-nbkpts-first <int> β€” Nb of break points for Bezier curve fitting (without localization) (int; default: 3000). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.sky-bspline-nbkpts-first [default = 3000].
  • --sky-bspline-nbkpts-second <int> β€” Nb of break points for Bezier curve fitting (with localization) (int; default: 3000). The full name of this option for the EsoRex configuration file is xsh.xsh_respon_slit_stare.sky-bspline-nbkpts-second [default = 3000].
  • --sky-bspline-order <int> β€” the order of the Bezier spline (int; default: 7). In the EsoRex config file the full name is xsh.xsh_respon_slit_stare.sky-bspline-order [default = 7]. πŸŽ€
  • --sky-bspline-niter <int> β€” number of iterations (int; default: 20). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-bspline-niter [default = 20].
  • --sky-bspline-kappa <float> β€” the kappa value used to kappa-sigma-clip the object (float; default: 5.0). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-bspline-kappa [default = 5.0].
  • --sky-method <str> β€” sky subtract method (BSPLINE, BSPLINE1, BSPLINE2 MEDIAN). Heads up bestie, BSPLINE is equivalent to BSPLINE1 (str; default: Β΄MEDIANΒ΄). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-method [default = MEDIAN].
  • --bspline-sampling <str> β€” BSPLINE sampling. UNIFORM uses the user defined nbkpts value, corrected for binning, for all orders. FINE multiplies the user defined nbkpts value, corrected for binning, by a hard coded coefficient optimized on each arm-order (str; default: Β΄FINEΒ΄). EsoRex config file full name: xsh.xsh_respon_slit_stare.bspline-sampling [default = FINE].
  • --sky-median-hsize <int> β€” half size of the running median, used if sky-method=MEDIAN (int; default: 20). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-median-hsize [default = 20].
  • --sky-slit-edges-mask <float> β€” size of the edges mask in arcsec (float; default: 0.5). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-slit-edges-mask [default = 0.5].
  • --sky-position1 <float> β€” central position of the sky window #1, in arcsec (float; default: 0.0). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-position1 [default = 0.0].
  • --sky-hheight1 <float> β€” half size of sky window #1, in arcsec (float; default: 0.0). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-hheight1 [default = 0.0].
  • --sky-position2 <float> β€” central position of the sky window #2, in arcsec (float; default: 0.0). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-position2 [default = 0.0].
  • --sky-hheight2 <float> β€” half size of the sky window #2, in arcsec (float; default: 0.0). EsoRex config file full name: xsh.xsh_respon_slit_stare.sky-hheight2 [default = 0.0].
  • --stdextract-interp-hsize <int> β€” half size of the mask used to define the object cross order profile (int; default: 30). EsoRex config file full name: xsh.xsh_respon_slit_stare.stdextract-interp-hsize [default = 30].
  • --do-optextract <bool> β€” TRUE if we do the optimal extraction (bool; default: False). EsoRex config file full name: xsh.xsh_respon_slit_stare.do-optextract [default = False].
  • --optextract-oversample <int> β€” oversample factor for the science image (int; default: 5). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-oversample [default = 5].
  • --optextract-box-half-size <int> β€” extraction box, in pixels (int; default: 10). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-box-half-size [default = 10].
  • --optextract-chunk-size <int> β€” chunk size, in bins (int; default: 50). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-chunk-size [default = 50].
  • --optextract-step-lambda <float> β€” lambda step, in nm (float; default: 0.02). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-step-lambda [default = 0.02].
  • --optextract-clip-kappa <float> β€” kappa for cosmics ray hits rejection (float; default: 3.0). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-clip-kappa [default = 3.0].
  • --optextract-clip-frac <float> β€” maximum bad pixels fraction for cosmics ray hits rejection (float; default: 0.4). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-clip-frac [default = 0.4].
  • --optextract-clip-niter <int> β€” maximum number of iterations for cosmics ray hits rejection (int; default: 2). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-clip-niter [default = 2].
  • --optextract-niter <int> β€” number of iterations (int; default: 1). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-niter [default = 1].
  • --optextract-method <str> β€” extraction method, GAUSSIAN | GENERAL (str; default: Β΄GAUSSIANΒ΄). EsoRex config file full name: xsh.xsh_respon_slit_stare.optextract-method [default = GAUSSIAN].
  • --correct-tellurics <bool> β€” TRUE if during response computation we apply telluric correction (bool; default: True). EsoRex config file full name: xsh.xsh_respon_slit_stare.correct-tellurics [default = True].
oh and also, bestie πŸ’œ 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. iykyk ✨

πŸ¦‹ SEE ALSO πŸ¦‹

The full documentation for the xshoo pipeline can be downloaded as a PDF file using the following URL:

ftp://ftp.eso.org/pub/dfs/pipelines/xshoo/xshoo-pipeline-manual-12.1.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 xshoo pipeline 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_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), xsh_wavecal(7). the whole friend group, honestly πŸ’…


⭐ VERSION ⭐

xsh_respon_slit_stare 3.5.3


πŸ‘‘ AUTHOR πŸ‘‘

P.Goldoni, L.Guglielmi, R. Haigron, F. Royer, D. Bramich, A. Modigliani <amodigli@eso.org > πŸ’–


πŸŽ€ BUG REPORTS πŸŽ€

Please report any problems to amodigli@eso.org . Alternatively, you may send a report to the ESO User Support Department usd-help@eso.org. they want to hear from u fr fr, don't just suffer in silence 🫢


🌸 LICENSE 🌸

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

yes bestie, the ALL CAPS WARRANTY bit is the legal version of "no promises, no cap" πŸ’€ but like, it's still free software and that's iconic ✨

and that's a wrap on xsh_respon_slit_stare version 3.5.3 of XSH_RESPON_SLIT_STARE(7) β€” go forth and sky-subtract responsibly, you absolute main character πŸŒŸπŸ’–πŸ¦‹

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