XSH_RESPON_SLIT_NOD(7)
β¨ XSH_RESPON_SLIT_NOD β¨
okay bestie, welcome to the XSH_RESPON_SLIT_NOD(7) page from the xshoo recipes manual π
yes the title is literally the whole vibe: XSH_RESPON_SLIT_NOD(7) on the left, xshoo recipes in the middle, XSH_RESPON_SLIT_NOD(7) again on the right, she's symmetrical, she's iconic, periodt.
πΈ NAME πΈ
xsh_respon_slit_nod β bestie this one reduces STD star frames when you're in SLIT configuration and nod mode π«Ά
π SYNOPSIS π
esorex xsh_respon_slit_nod [OPTIONS] FILE.sof
no cap, that's the whole summoning ritual: call esorex, hand her the recipe name, maybe some [OPTIONS], and a FILE.sof to chew on π
π¦ DESCRIPTION π¦
okay so real talk: this recipe reduces science exposure in SLIT configuration and NOD mode β¨ like that's her whole job, that's her main character energy.
π Input Frames :
she's not low-maintenance, she has a whole checklist. here's what she wants sliding into her .sof:
- A set of n Science frames ( n even ), Tag =
OBJECT_SLIT_NOD_armβ yes the count has to be even, she's not doing math on an odd number, that's the rules π₯ - Spectral format table (Tag =
SPECTRAL_FORMAT_TAB_arm) [UVB,VIS]A master bias frame (Tag =MASTER_BIAS_arm) β note the lil bracket situation: UVB and VIS only, okay? π- A master flat frame (Tag =
MASTER_FLAT_SLIT_arm) - An order table frame (Tag =
ORDER_TABLE_EDGES_SLIT_arm) [poly mode]A wave solution frame (Tag =WAVE_TAB_2D_arm)[poly mode]A wave map frame (Tag =WAVE_MAP_arm)[poly mode]A disp table frame (Tag =DISP_TAB_arm)[physical model mode]A model cfg table (Format =TABLE, Tag =XSH_MOD_CFG_TAB_arm)[OPTIONAL]A telluric model catalog (Tag =TELL_MOD_CAT_armarm=VIS,NIR) β optional bestie, but she'll take it if you've got it π- A standard star fluxes catalog (Tag =
FLUX_STD_CATALOG_armType =FLX) - A table to set response sampling points (Tag =
RESP_FIT_POINTS_CAT_arm) [OPTIONAL]An atmospheric extinction table (Tag =ATMOS_EXT_arm) β and okay, listen: if provided this is the one used to flux calibrate the spectra. like, it overrides, it's the chosen one, no cap π
π Products :
and here's what she gives you back, the whole glow-up lineup:
[If STD is in catal]The response function (Tag =PREFIX_RESPONSE_ORDER1D_SLIT_arm)[If STD is in catal]The response function (Tag =PREFIX_RESPONSE_MERGE1D_SLIT_arm)PREFIX_ORDER2D_arm(2 dimension)PREFIX_ORDER1D_arm(1 dimension)PREFIX_MERGE2D_arm(2 dimension)PREFIX_MERGE1D_arm(1 dimension)PREFIX_WAVE_MAP_arm, wave map imagePREFIX_SLIT_MAP_arm, slit map image[If STD is in catal]Flux calibrated order-by-order 2D spectrum (Tag =PREFIX_FLUX_ORDER2D_arm)[If STD is in catal]Flux calibrated order-by-order 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)
and then the lil plot twist about that PREFIX thing: where PREFIX is SCI, FLUX, TELL if input raw DPR.TYPE contains OBJECT or FLUX or TELLURIC π§ so she's literally picking her own name based on the vibes of the input, iykyk.
more coming bestie, hold on π
β¨ OPTIONS β¨
okay bestie, this is the part where we go through EVERY. SINGLE. KNOB. ποΈ no skimming, no "you'll figure it out" β we're listing all of them, and every one of them has a full name for the EsoRex config file so you can go write your own config and be that girl. π
--keep-temp <str>β if you set it tono, the temporary files get yeeted. (str; default:no). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.keep-temp [default = no].--debug-level <str>β extra xshooter debug level, and it has to be one ofnone,low,medium,high. (str; default:none). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.debug-level [default = none].--time-stamp <bool>β throws a timestamp onto the product file name, so your outputs don't all look like twins. (bool; default: False). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.time-stamp [default = False].--decode-bp <int>β the integer version of the bits that count as bad when it's decoding the bad pixel mask pixel values. the codes you'll actually bump into: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: 1741684735). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.decode-bp [default = 1741684735].--pre-overscan-corr <int>β the pre-overscan correction vibe check.0: no correction,1: mean overscan correction,2: mean prescan correction,3: (mean pre+mean overscan)/2 correction. (int; default: 1). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.pre-overscan-corr [default = 1].--stack-method <str>β the method used to build the master frame. (str; default:median). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.stack-method [default = median].--klow <float>β the kappa used to clip low level values, and it only matters when the method is set tomean. (float; default: 5.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.klow [default = 5.0].--khigh <float>β the kappa used to clip high level values, again only when the method is set tomean. (float; default: 5.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.khigh [default = 5.0].--removecrhsingle-sigmalim <float>β the Poisson fluctuation threshold used to flag CRHs (go read van Dokkum, PASP,113,2001,p1420-27, it's giving academic). (float; default: 20.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.removecrhsingle-sigmalim [default = 20.0].--removecrhsingle-flim <float>β the minimum contrast between the Laplacian image and the fine structure image that a point needs to have before it gets flagged as a CRH (again, van Dokkum, PASP,113,2001,p1420-27). (float; default: 2.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.removecrhsingle-flim [default = 2.0].--removecrhsingle-niter <int>β max number of iterations, literally just that. (int; default: 4). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.removecrhsingle-niter [default = 4].--rectify-kernel <str>β the name of the interpolation kernel used, and your options are:tanh,sinc,sinc2,lanczos,hamming,hann. (str; default:tanh). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.rectify-kernel [default = tanh].--rectify-radius <float>β the rectify interpolation radius, measured in bin units. (float; default: 2.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.rectify-radius [default = 2.0].--rectify-bin-lambda <float>β wavelength step in the output spectrum, in nm. (float; default: -1.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.rectify-bin-lambda [default = -1.0].--rectify-bin-slit <float>β spatial step along the slit in the output spectrum, in arcsec. (float; default: -1.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.rectify-bin-slit [default = -1.0].--rectify-fast <bool>β fast if TRUE, whereRect[B-A] = -Rect[A-B], and in that case only entire pixel shifts get applied. (bool; default: True). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.rectify-fast [default = True].--localize-method <str>β the localization method used to detect the object centroid and height on the slit:MANUAL,MAXIMUM,GAUSSIAN. (str; default:MANUAL). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-method [default = MANUAL].--localize-chunk-nb <int>β how many chunks in the full spectrum are used to localize the object. (int; default: 10). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-chunk-nb [default = 10].--localize-thresh <float>β the threshold relative to the peak intensity, below which the edges of the object get detected forMAXIMUMlocalization. (float; default: 0.1). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-thresh [default = 0.1].--localize-deg-lambda <int>β the degree in lambda in the localization polynomial expressionslit=f(lambda), and it's only used forMAXIMUMandGAUSSIAN. (int; default: 0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-deg-lambda [default = 0].--localize-slit-position <float>β object position on the slit forMANUALlocalization, in arcsec. (float; default: 0.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-slit-position [default = 0.0].--localize-slit-hheight <float>β object half height on the slit forMANUALlocalization, in arcsec. (float; default: 2.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-slit-hheight [default = 2.0].--localize-kappa <float>β the kappa value used for sigma clipping in the localization polynomial fit. (float; default: 3.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-kappa [default = 3.0].--localize-niter <int>β how many iterations of sigma clipping happen in the localization polynomial fit. (int; default: 3). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-niter [default = 3].--localize-use-skymask <bool>β TRUE if we wanna mask sky lines using theSKY_LINE_LISTfile. (bool; default: False). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-use-skymask [default = False].--localize-nod-throw <float>β the step (arcsec) between the A and B images in nodding mode. (float; default: 0.0). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.localize-nod-throw [default = 0.0].--extract-method <str>β the method used for extraction:LOCALIZATION,NOD. (str; default:NOD). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.extract-method [default = NOD].--stdextract-interp-hsize <int>β half size of the mask used to define the object cross order profile. (int; default: 30). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.stdextract-interp-hsize [default = 30].--combinenod-throwlist <str>β name of the ascii file holding the list of throw shifts with respect to the first exposure. (str; default:throwlist.asc). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.combinenod-throwlist [default = throwlist.asc].--combinenod-method <str>β the combination method for nodded frames:MEDIAN,MEAN. (str; default:MEAN). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.combinenod-method [default = MEAN].--max-slit <float>β Lower Slit Limit (localize and extract. yes, that's exactly how it reads, we're keeping it. (float; default: 5.7). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.max-slit [default = 5.7].--min-slit <float>β Upper Slit Limit (localize and extract. same energy, same dangling paren. (float; default: -5.3). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.min-slit [default = -5.3].--correct-tellurics <bool>β TRUE if we apply telluric correction during the response computation. (bool; default: True). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.correct-tellurics [default = True].--correct-sky-by-median <bool>β TRUE if the resampled spectrum at each wavelength gets median subtracted to remove sky lines. (bool; default: True). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.correct-sky-by-median [default = True].--scale-combine-nod-method <int>β frame scaling when nod frames are combined:0(no-scaling);1(scaling). (int; default: 1). full name in the EsoRex config file isxsh.xsh_respon_slit_nod.scale-combine-nod-method [default = 1].
π«Ά and yes, bestie, you can absolutely make a configuration file holding all these options plus whatever default values you like. the details live in what the esorex --help command tells you. go look. it's giving self-sufficient. π
π SEE ALSO π
okay bestie, here's the β¨ extended universe β¨ of this recipe β the full tea:
- The complete documentation for the xshoo pipeline can be downloaded as a PDF file from this URL right here:
ftp://ftp.eso.org/pub/dfs/pipelines/xshoo/xshoo-pipeline-manual-12.1.pdf
- Wanna see the whole landscape of ESO pipelines? There's a web page for that, and it's giving directory-of-everything:
https://www.eso.org/sci/software/pipelines/
- The basic lore on the EsoRex program lives in the
esorex(1) man page. go read it, it's the parent figure here π«Ά - And yes, you can call the pipelines from python using the python-cpl package π β more info lives here:
https://packages.python.org/python-cpl/index.html
- The other recipes of the xshoo pipeline, aka the whole friend group, no cap:
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_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)xsh_wavecal(7)
β VERSION β
xsh_respon_slit_nod 3.5.3 π
π AUTHOR π
P.Goldoni, L.Guglielmi, R. Haigron, F. Royer, D. Bramich A. Modigliani <amodigli@eso.org>
(these are the icons who made it happen, we stan π)
π¨ BUG REPORTS π¨
found a bug? bestie, please don't suffer in silence π β report any problems to amodigli@eso.org.
Alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>. two whole doors, pick your fav π«Ά
π LICENSE π
okay so legally speaking β here's the whole thing, every word, no skipping:
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. 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., 59 Temple Place, Suite 330, Boston, MA 02111-1307 USA
and that's a wrap on xsh_respon_slit_nod, bestie π¦β¨ this is page xsh_respon_slit_nod, version 3.5.3, and it's filed under XSH_RESPON_SLIT_NOD(7) β aka the man page title itself π go forth and reduce them nodding slits, you got this π
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