MUSE_CREATE_SKY(7)
π« muse_create_sky β the night sky, but make it a recipe π«
okay bestie, so this is a muse pipeline recipe β it lives in section 7 of the manual, and honestly? it's giving "look at the empty sky and turn it into a model" energy. no cap. β¨
π NAME π
muse_create_sky β literally builds a night sky model out of selected pixels from an exposure of empty sky. π¦
like. you point at nothing (well, mostly nothing), and you get back the sky. iconic behavior fr fr.
π SYNOPSIS π
esorex muse_create_sky [OPTIONS] FILE.sof
that's it, that's the whole vibe. a .sof file, some options, and we're off. π
β¨ DESCRIPTION β¨
so what does this recipe actually do, you ask? πΈ
It creates the continuum and the atmospheric transition line spectra of the night sky. Where does it get them from? From the data in a pixel table(s) that belongs to one exposure of (mostly) empty sky. π
one exposure. mostly empty. and it pulls the sky out of it. main character energy honestly. π
π OPTIONS π
bestie, there are nine of them. all of them matter. no skipping. let's go one by one, i'll hold your hand. π«Ά
--fraction <float>β This is how much of the image (not counting the ignored part) gets treated as sky. If you handed in a sky mask, the fraction applies to the regions inside the mask. And if you want the whole sky mask used, set this thing to1. It's a float, and it defaults to0.75. The full name for the EsoRex configuration file ismuse.muse_create_sky.fraction[default =0.75].--ignore <float>β The fraction of the image that gets ignored. Same mask rule as above: if there's an input sky mask, the fraction applies to the regions within the mask. Want the whole sky mask? Set this to0. It's a float, default0.05. Full EsoRex config name:muse.muse_create_sky.ignore[default =0.05].--sampling <float>β The spectral sampling of the sky spectrum, in Angstrom. Float, default0.3125. Full EsoRex config name:muse.muse_create_sky.sampling[default =0.3125].--csampling <float>β The spectral sampling of the continuum spectrum, also in Angstrom. Float, default0.3125. Full EsoRex config name:muse.muse_create_sky.csampling[default =0.3125].--crsigma <str>β Sigma level clipping for both cube-based and spectrum-based CR rejection. Okay so this one has rules: it has to be a string of two comma-separated floating-point numbers. The first value = the sigma-level rejection for cube-based CR rejection (using"median", seemuse_scipost). The second value = the sigma-level for spectrum-based CR cleaning. And here's the cute part: you can switch both off by passing zero or a negative value. It's a string, defaultΒ΄15.,15.Β΄. Full EsoRex config name:muse.muse_create_sky.crsigma[default =15.,15.].--lambdamin <float>β Cuts off the data below this wavelength, after loading the pixel table(s). Float, default4000.0. Full EsoRex config name:muse.muse_create_sky.lambdamin[default =4000.0].--lambdamax <float>β Cuts off the data above this wavelength, also after loading the pixel table(s). Float, default10000.0. Full EsoRex config name:muse.muse_create_sky.lambdamax[default =10000.0].--lambdaref <float>β The reference wavelength used for correcting differential atmospheric refraction. Here's the tea: the R-band (peak wavelength ~7000Angstrom), which is usually what's used for guiding, sits close to the central wavelength of MUSE β so if you don't know anything else, use7000.0Angstrom. And if you pass a value less than zero, that switches DAR correction off. Float, default7000.0. Full EsoRex config name:muse.muse_create_sky.lambdaref[default =7000.0].
okay real talk for a sec π«Ά β you can make a configuration file holding all these options plus suitable default values. For the deets on that, go check what esorex --help tells you. no cap.
π₯ SEE ALSO π₯
the full documentation for the muse pipeline can be downloaded as a PDF, bestie, right here:
ftp://ftp.eso.org/pub/dfs/pipelines/muse/muse-pipeline-cookbook-2.8.7.pdf
an overview of all the existing ESO pipelines lives at:
https://www.eso.org/sci/software/pipelines/
basic documentation about the EsoRex program itself? that's at the esorex (1) man page. πΈ
and fun fact β you can call the pipelines from python using the python-cpl package. more info at:
https://packages.python.org/python-cpl/index.html
now, the other recipes of the muse pipeline β and yes i'm listing every single one because they're all stars β:
muse_ampl(7), muse_astrometry(7), muse_bias(7), muse_dark(7), muse_exp_align(7), muse_exp_combine(7), muse_flat(7), muse_geometry(7), muse_illum(7), muse_lingain(7), muse_lsf(7), muse_qi_mask(7), muse_scibasic(7), muse_scipost(7), muse_scipost_apply_astrometry(7), muse_scipost_calibrate_flux(7), muse_scipost_combine_pixtables(7), muse_scipost_correct_dar(7), muse_scipost_correct_rv(7), muse_scipost_make_cube(7), muse_scipost_raman(7), muse_scipost_subtract_sky(7), muse_scipost_subtract_sky_simple(7), muse_standard(7), muse_twilight(7), muse_wavecal(7)
π§ VERSION π§
muse_create_sky 2.8.7
π AUTHOR π
Ole Streicher <https://support.eso.org>
π BUG REPORTS π
please report any problems to <https://support.eso.org>. alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>.
(they're nice, i promise. don't be shy.)
π LICENSE π
this file is part of the MUSE Instrument Pipeline Copyright (C) 2005, 2019 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., 51 Franklin St, Fifth Floor, Boston, MA 02111-1307 USA
π and that's the whole page, bestie. go model yourself some sky.
muse_create_sky version 2.8.7, dated 2.8.7, from the MUSE pipeline β mwah, slay, bye. πβ¨ππ¦πΈπ π«Ά
π¦ where this page comes from
- debian bookworm: cpl-plugin-muse-doc 2.8.7+dfsg-3 Β· GPL-v2+
- ubuntu noble: cpl-plugin-muse-doc 2.8.7+dfsg-3 Β· GPL-v2+
- π girlified by deepseek-ai/DeepSeek-V4.1-Flash on : a language model's rewrite of the original, under its terms