FLAMES_CAL_MKMASTER(7)

📦
version 6.1.8 · 2 versions
, in debian bookworm, ubuntu noble

💖 FLAMES_CAL_MKMASTER 💖

okay bestie, gather round, because this is flames_cal_mkmaster from the uves recipes manual (that's the FLAMES_CAL_MKMASTER(7) page, section 7, iykyk). It's the recipe that builds you a master flat frame so your FIBER mode data reduction doesn't fall apart. Let's get into it 🦋

✨ NAME ✨

flames_cal_mkmaster — creates a master flat frame to support FIBER mode data reduction

🌸 SYNOPSIS 🌸

esorex flames_cal_mkmaster [OPTIONS] FILE.sof

💅 DESCRIPTION 💅

So this recipe makes a composite master flat frame to reduce FIBER mode data, and the way it does that is honestly giving organized:

  1. It groups each input raw flat frame per grating setting. Then for each set:
    1. subtracts the master bias frame from each flat field frame,
    2. divides each flat field frame by the exposure time for that frame,
    3. takes the median of all bias subtracted, normalized raw flat frames,
    4. optionally subtracts the master dark frame, and
    5. subtracts the background to get the bias subtracted, optionally dark subtracted, normalized, background subtracted master flat-field frame.
  2. It creates a synthetic master frame resulting from the coaddition of each master flat frame obtained by each set. Symbolically,
masterflat = median( (flat_i - masterbias)/exptime_i ) - masterdark/exptime
            - background.

The input flat field frames must have same tag which must match (SFLAT_(BLUE|RED), for example SFLAT_BLUE or FLAT_RED. Also, a master bias (MASTER_BIAS_xxxx) and ordertable (ORDER_TABLE_xxxx) must be provided for each chip (xxxx = BLUE, REDL, REDU). A master dark frame (MASTER_(P)DARK_xxxx) may optionally be provided. On blue input the recipe computes one master flat field frame; on red input the recipe produces a master flat field frame for each chip (MASTER_SFLAT_xxxx).

bestie pls note: the matching-tag thing and the per-chip master bias + ordertable requirement are not optional, they're the vibe check your data has to pass 🫶

🎀 OPTIONS 🎀

  • --backsub.mmethod <str> — the background measuring method. If it's equal to ´median´ the background is sampled using the median of a subwindow. If ´minimum´, the subwindow minimum value is used. If ´no´, no background subtraction is done at all. (str; default: ´median´). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.backsub.mmethod [default = median].
  • --backsub.npoints <int> — this is the number of columns in interorder space used to sample the background. (int; default: 82). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.backsub.npoints [default = 82].
  • --backsub.radiusy <int> — the height (in pixels) of the background sampling window is (2*radiusy + 1). This parameter is not corrected for binning, no cap. (int; default: 2). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.backsub.radiusy [default = 2].
  • --backsub.sdegree <int> — degree of interpolating splines. Currently only degree = 1 is supported (int; default: 1). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.backsub.sdegree [default = 1].
  • --backsub.smoothx <float> — if spline interpolation is used to measure the background, the x-radius of the post-smoothing window is (smoothx * image_width). Here, ´image_width´ is the image width after binning. If negative, the default values are used: (25.0/4096) for blue flat-field frames, (50.0/4096) for red flat-field frames, (300.0/4096) for blue science frames and (300.0/4096) for red science frames. (float; default: -1.0). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.backsub.smoothx [default = -1.0].
  • --backsub.smoothy <float> — if spline interpolation is used to measure the background, the y-radius of the post-smoothing window is (smoothy * image_height). Here, ´image_height´ is the image height after binning. If negative, the default values are used: (100.0/2048) for blue flat-field frames, (300.0/2048) for red flat-field frames, (200.0/2048) for blue science frames and (500.0/2048) for red science frames. (float; default: -1.0). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.backsub.smoothy [default = -1.0].
  • --debug <bool> — whether or not to save intermediate results to local directory (bool; default: False). The full name of this option for the EsoRex configuration file is uves.debug [default = False].
  • --norm_method <str> — method used to build master frame (str; default: ´exptime´). The full name of this option for the EsoRex configuration file is flames_cal_mkmaster.norm_method [default = exptime].
  • --plotter <str> — any plots produced by the recipe are redirected to the command specified by this parameter. The plotting command must contain the substring ´gnuplot´ and must be able to parse gnuplot syntax on its standard input. Valid examples of such a command may include ´gnuplot -persist´ and ´cat > mygnuplot$$.gp´. A finer control of the plotting options can be obtained by writing an executable script, e.g. my_gnuplot.pl, that executes gnuplot after setting the desired gnuplot options (e.g. set terminal pslatex color). To turn off plotting, set this parameter to ´no´ (str; default: ´no´). The full name of this option for the EsoRex configuration file is uves.plotter [default = no].
  • --process_chip <str> — for RED arm data process the redl, redu, or both chip(s) (str; default: ´both´). The full name of this option for the EsoRex configuration file is uves.process_chip [default = both].

Note that 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.

🔥 SEE ALSO 🔥

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

ftp://ftp.eso.org/pub/dfs/pipelines/uves/uves-pipeline-manual-6.1.8.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 uves pipeline are:

⭐ VERSION ⭐

flames_cal_mkmaster 6.1.8

👑 AUTHOR 👑

Andrea Modigliani <cpl@eso.org>

🙈 BUG REPORTS 🙈

Please report any problems to cpl@eso.org. Alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>.

bestie if it breaks, do NOT suffer in silence, tell the ESO girlies 💀

🌈 LICENSE 🌈

This file is part of the FLAMES/UVES Pipeline Copyright (C) 2004, 2005, 2006, 2007 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

aaaand that's the whole page, bestie 🧚✨ no details skipped, every flag accounted for, we ate 💅 This was flames_cal_mkmaster version 6.1.8, straight out of the uves recipes era — go forth and make that master flat, you've got this 🍓💖

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