SYNOPSISesorex kmo_sky_mask [OPTIONS] FILE.sof
DESCRIPTIONThis recipes calculates masks of the skies surrounding the objects in the diff- erent IFUs of a reconstructed F3I frame. In the resulting mask pixels belonging to objects have value 1 and sky pixels have value 0.
The noise and the background level of the input data cube are estimated using the mode calculated in kmo_stats. If the results aren't satisfactory, try chan- ging --cpos_rej and --cneg_rej. Then pixels are flagged in the data cube which have a value less than the mode plus twice the noise (val < mode + 2*sigma).
For each spatial pixel the fraction of flagged pixels in its spectral channel is determined.
Spatial pixels are selected where the fraction of flagged spectral pixels is greater than 0.95 (corresponding to the 2*sigma above).
The input cube can contain noise extensions, but they will be ignored. The out- put doesn’t contain noise extensions.
BASIC PARAMETERS--fraction The fraction of pixels that have to be greater than the threshold can be defi- ned with this parameter (value must be between 0 and 1).
--range If required, a limited wavelength range can be defined (e.g. "1.8,2.1").
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
val < mean - stdev * cneg_rej In the first iteration median and percentile level are used.
category Type Explanation Required #Frames
-------- ----- ----------- -------- -------
<none or any> F3I The datacube frame Y 1
category Type Explanation
-------- ----- -----------
SKY_MASK F2I The mask frame
- --range <str>
- Min & max wavelengths to use in sky pixel determination, e.g. [x1_start,x1_end] (microns). (str; default: ''). The full name of this option for the EsoRex configuration file is kmos.kmo_sky_mask.range [default = ].
- --fraction <float>
- Minimum fraction of spatial pixels to select as sky (value between 0 and 1). (float; default: 0.95). The full name of this option for the EsoRex configuration file is kmos.kmo_sky_mask.fraction [default = 0.95].
- --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_sky_mask.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_sky_mask.cneg_rej [default = 3.0].
- --citer <long>
The number of iterations for kappa-sigma-clipping. (long; default: 3). The full name of this option for the EsoRex configuration
file is kmos.kmo_sky_mask.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.
AUTHORAlex Agudo Berbel <[email protected]>
BUG REPORTSPlease report any problems to [email protected] Alternatively, you may send a report to the ESO User Support Department <[email protected]>.
LICENSEThis 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