FLAMES_CAL_MKMASTER(7) | uves recipes | FLAMES_CAL_MKMASTER(7) |
flames_cal_mkmaster - Creates a master flat frame to support FIBER mode data reduction
esorex flames_cal_mkmaster [OPTIONS] FILE.sof
This recipe creates a composite master flat frame to reduce FIBER mode data by: 1) Group each input raw flat frame per grating setting. Then for each set: 1a) subtracts the master bias frame from each flat field frame, 1b) divides each flat field frame by the exposure time for that frame, 1c) takes the median of all bias subtracted, normalized raw flat frames, 1d) optionally subtracts the master dark frame, and 1e) subtracts the background to get the bias subtracted, optionally dark subtracted, normalized, background subtracted master flat-field frame.
2) 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).
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.
The full documentation for the uves pipeline can be downloaded as a PDF file using the following URL:
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 flames_cal_orderpos(7), flames_cal_predict(7), flames_cal_prep_sff_ofpos(7), flames_cal_wavecal(7), flames_obs_redchain(7), flames_obs_scired(7), flames_utl_unpack(7), uves_cal_cd_align(7), uves_cal_mbias(7), uves_cal_mdark(7), uves_cal_mflat(7), uves_cal_mflat_combine(7), uves_cal_mkmaster(7), uves_cal_orderpos(7), uves_cal_predict(7), uves_cal_response(7), uves_cal_tflat(7), uves_cal_wavecal(7), uves_obs_redchain(7), uves_obs_scired(7), uves_utl_ima_arith(7), uves_utl_remove_crh_single(7)
flames_cal_mkmaster 6.1.8
Andrea Modigliani <cpl@eso.org>
Please report any problems to cpl@eso.org. Alternatively, you may send a report to the ESO User Support Department <usd-help@eso.org>.
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
6.1.8 | flames_cal_mkmaster |