Provided by: cpl-plugin-kmos-doc_2.1.0+dfsg-1_all
kmo_stats - Perform basic statistics on a KMOS-conform fits-file
esorex kmo_stats [OPTIONS] FILE.sof
This recipe performs basic statistics on KMOS-conform data-frames of type F2D, F1I, F2I and F3I either with or without noise and RAW. Optionally a 2D mask can be provided to define a region on which the statistics should be calculated on (mask 0: exclude pixel, mask 1: include pixel). A mask can’t be provided for statistics on F1I frames. The output is stored in a vector of length 11. The vector represents following values: 1. Number of pixels 2. Number of finite pixels 3. Mean 4. Standard Deviation 5. Mean with iterative rejection (i.e. mean & sigma are calculated iterati- vely, each time rejecting pixels more than +/-N sigma from the mean) 6. Standard Deviation with iterative rejection 7. Median 8. Mode (i.e. the peak in a histogram of pixel values) 9. Noise (a robust estimate given by the standard deviation from the nega- tive side of the histogram of pixel values) 10. Minimum 11. Maximum The same numerical operations are applied to the noise as with the data itself. BASIC PARAMETERS --ext These parameters specify with extensions to process. The value 0, which is default, calulates all extensions. ADVANCED PARAMETERS --cpos_rej --cneg_rej --citer An iterative sigma clipping is applied in order to calculate the mode (using kmo_stats). For each position all pixels in the spectrum are examined. If they deviate significantly, they will be rejected according to the conditions: val > mean + stdev * cpos_rej and val < mean - stdev * cneg_rej In the first iteration median and percentile level are used. Input files: DO DO KMOS category group Type Explanation Required #Frames -------- ----- ----- ----------- -------- ------- <none or any> - F3I or The datacubes Y 1 F2I or F1I or F2D or B2D or RAW <none or any> - F2I or The mask N 0,1 F2D or B2D or RAW Output files: DO KMOS category Type Explanation -------- ----- ----------- STATS F1I Calculated statistics parameters
--ext <int> The extension the stats should be calculated of. Zero is default and calculates the stats of all extensions (int; default: 0). The full name of this option for the EsoRex configuration file is kmos.kmo_stats.ext [default = 0]. --cpos_rej <float> The positive rejection threshold for kappa-sigma-clipping (sigma). (float; default: 3.0). The full name of this option for the EsoRex configuration file is kmos.kmo_stats.cpos_rej [default = 3.0]. --cneg_rej <float> The negative rejection threshold for kappa-sigma-clipping (sigma). (float; default: 3.0). The full name of this option for the EsoRex configuration file is kmos.kmo_stats.cneg_rej [default = 3.0]. --citer <int> The number of iterations for kappa-sigma-clipping. (int; default: 3). The full name of this option for the EsoRex configuration file is kmos.kmo_stats.citer [default = 3]. 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 kmos pipeline can be downloaded as a PDF file using the following URL: ftp://ftp.eso.org/pub/dfs/pipelines/kmos/kmos-pipeline-manual-2.9.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 kmos pipeline are kmo_arithmetic(7), kmo_copy(7), kmo_fit_profile(7), kmo_fits_strip(7), kmo_make_image(7), kmo_noise_map(7), kmo_rotate(7), kmo_shift(7), kmo_sky_mask(7), kmos_combine(7), kmos_dark(7), kmos_extract_spec(7), kmos_flat(7), kmos_gen_reflines(7), kmos_gen_telluric(7), kmos_illumination(7), kmos_reconstruct(7), kmos_sci_red(7), kmos_sky_tweak(7), kmos_std_star(7), kmos_test(7), kmos_wave_cal(7)
Alex Agudo Berbel <firstname.lastname@example.org>
Please report any problems to email@example.com. Alternatively, you may send a report to the ESO User Support Department <firstname.lastname@example.org>.
This file is part of the CRIRES Instrument Pipeline Copyright (C) 2002,2003 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