HAWKI_SCIENCE_POSTPROCESS(7)
π hawki_science_postprocess(7) π
okay bestie, this is the manual page for hawki_science_postprocess, one of the hawki recipes. sit down, grab a strawberry π, and let's get into it.
β¨ NAME β¨
hawki_science_postprocess β the HAWKI post processing recipe. yes that's the whole name. iconic, lowkey.
π¦ SYNOPSIS π¦
esorex hawki_science_postprocess [OPTIONS] FILE.sof
that's it. that's the whole vibe check.
πΈ DESCRIPTION πΈ
so hawki_science_postprocess is literally the HAWKI science post processing recipe, no cap.
what it does: it postprocesses a stacked pawprint for HAWKI data. it forms a filled tile, then photometrically and astrometrically calibrates that tiled image. optionally β if you're feeling spicy β it can nebulise the stacked images before source detection. main character energy fr fr.
π what files it wants in the SOF
the program accepts the following files in the SOF:
BASIC_CALIBRATED_SCIβ a set of processed images from a jitter sequenceBASIC_VAR_MAPβ a variance map for each sequence imageMASTER_CONFβ a master confidence map for the jitter sequencePHOTCAL_TABβ a photometric calibration tableMASTER_2MASS_CATALOGUE_ASTROMβ a master 2MASS index for astrometry, orMASTER_PPMXL_CATALOGUE_ASTROMβ a master PPMXL index for astrometry, orMASTER_LOCAL_CATALOGUE_ASTROMβ a master local astrometric FITS fileMASTER_2MASS_CATALOGUE_PHOTOMβ a master 2MASS index for photometry, orMASTER_PPMXL_CATALOGUE_PHOTOMβ a master PPMXL index photometry, orMASTER_LOCAL_CATALOGUE_PHOTOMβ a master local photometric FITS fileMATCHSTD_PHOTOMβ a master photometric matched stds catalogue (optional)SCHLEGEL_MAP_NORTHβ Northern Schlegel MapSCHLEGEL_MAP_SOUTHβ Southern Schlegel Map
π«Ά heads up bestie: all of the above are required unless specified otherwise. the astrometric and photometric files are not required if these can be obtained from the CDS using the --cdssearch options. so like, you have options. slay.
π OPTIONS π
sixteen of them. every single one. let's go π
--nebulise<bool> β nebulise the stacks before object detection? (bool; default:False). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.nebulise[default =False].--minphotom<int> β minimum number of stars for photometry solution (int; default:20). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.minphotom[default =20].--prettynames<bool> β use pretty product names? (bool; default:False). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.prettynames[default =False].--cdssearch_astrom<str> β CDS astrometric catalogue (str; default:none). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cdssearch_astrom[default =none].--cdssearch_photom<str> β CDS photometric catalogue (str; default:none). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cdssearch_photom[default =none].--stk_fast<str> β use fast stacking? (str; default:auto). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.stk_fast[default =auto].--stk_nfst<int> β Nframes before we switch to slow stack algorithm (int; default:30). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.stk_nfst[default =30].--savemstd<bool> β save matched standard catalogues? (bool; default:False). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.savemstd[default =False].--neb_medfilt<int> β median filter size for nebuliser (int; default:101). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.neb_medfilt[default =101].--neb_linfilt<int> β linear filter size for nebuliser (int; default:33). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.neb_linfilt[default =33].--cat_ipix<int> β minimum pixel area for each detected object (int; default:4). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cat_ipix[default =4].--cat_thresh<float> β detection threshold in sigma above sky (float; default:2.5). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cat_thresh[default =2.5].--cat_icrowd<bool> β use deblending? (bool; default:True). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cat_icrowd[default =True].--cat_rcore<float> β value of Rcore in pixels (float; default:10.0). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cat_rcore[default =10.0].--cat_nbsize<int> β background smoothing box size (int; default:64). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cat_nbsize[default =64].--cacheloc<str> β location for standard star cache (str; default:.). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.cacheloc[default =.].--magerrcut<float> β cut in magnitude error (float; default:100.0). the full name of this option for the EsoRex configuration file ishawki.hawki_science_postprocess.magerrcut[default =100.0].
π‘ oh also β 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. you're welcome π«Ά
π SEE ALSO π
the full documentation for the hawki pipeline can be downloaded as a PDF file using the following URL:
ftp://ftp.eso.org/pub/dfs/pipelines/hawki/hawki-pipeline-manual-2.4.11.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 hawki pipeline are:
hawki_cal_dark(7)hawki_cal_distortion(7)hawki_cal_flat(7)hawki_cal_zpoint(7)hawki_dark_combine(7)hawki_detector_noise(7)hawki_linearity_analyse(7)hawki_sci_jitter(7)hawki_science_process(7)hawki_standard_process(7)hawki_step_apply_dist(7)hawki_step_basic_calib(7)hawki_step_combine(7)hawki_step_compute_bkg(7)hawki_step_detect_obj(7)hawki_step_photom_2mass(7)hawki_step_refine_offsets(7)hawki_step_stats(7)hawki_step_stitch(7)hawki_step_subtract_bkg(7)hawki_tec_filtchk(7)hawki_twilight_flat_combine(7)hawki_util_gendist(7)hawki_util_stdstars(7)
β VERSION β
hawki_science_postprocess 2.4.11
π§ AUTHOR π§
Jim Lewis <jrl@ast.cam.ac.uk>
π BUG REPORTS π
please report any problems to jrl@ast.cam.ac.uk. alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>. they're nice, they got you π«Ά
π LICENSE π
this file is part of the HAWKI Instrument Pipeline Copyright (C) 2015 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 this was hawki_science_postprocess 2.4.11, from the hawki recipes, and yes β she ate. periodt. β¨π¦π
πΈπ
π¦ where this page comes from
- debian bookworm: cpl-plugin-hawki-doc 2.4.11+dfsg-1 Β· GPL-v2+
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- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms