The visir_old_spc_wcal recipe¶
- visir_old_spc_wcal¶
Synopsis¶
Old DRS detector: Spectroscopic wavelength calibration recipe
Description¶
This recipe estimates the dispersion relation using the atmospheric spectrum in a long-slit spectroscopy half-cycle frame.
The files listed in the Set Of Frames (sof-file) must be tagged: VISIR-Long-Slit-Spectroscopy-file.fits SPEC_CAL_LMR_WCAL VISIR-Quantum-Efficiency-Calibration-file.fits SPEC_CAL_QEFF VISIR-Atmospheric-Emission-Lines-Calibration-file.fits SPEC_CAL_LINES
Additionally, a bad pixel map with a PRO.CATG of SPEC_BPM may be added to the Set Of Frames with tag: BPM.
Constructor¶
- cpl.Recipe("visir_old_spc_wcal")
Create an object for the recipe visir_old_spc_wcal.
import cpl
visir_old_spc_wcal = cpl.Recipe("visir_old_spc_wcal")
Parameters¶
- visir_old_spc_wcal.param.auto_bpm¶
Automatic detection and correction of bad pixels (bool; default: True) [default=True].
- visir_old_spc_wcal.param.plot¶
The recipe can produce a number of predefined plots. Zero means that none of the plots are produced, while increasing values (e.g. 1 or 2) increases the number of plots produced. If the plotting fails a warning is produced, and the recipe continues. The default behaviour of the plotting is to use gnuplot (with option -persist). The recipe currently produces 1D-plots using gnuplot commands. The recipe user can control the actual plotting-command used by the recipe to create the plot by setting the environment variable CPL_PLOTTER. Currently, if CPL_PLOTTER is set it must contain the string ‘gnuplot’. Setting it to ‘cat > my_gnuplot_$$.txt’ causes a number of ASCII-files to be created, which each produce a plot when given as standard input to gnuplot (e.g. later or on a different computer). 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) and then setting CPL_PLOTTER to my_gnuplot.pl. The predefined plots include plotting of images. Images can be plotted not only with gnuplot, but also using the pnm format. This is controlled with the environment variable CPL_IMAGER. If CPL_IMAGER is set to a string that does not contain the word gnuplot, the recipe will generate the plot in pnm format. E.g. setting CPL_IMAGER to ‘display - &’ will produce a gray-scale image using the image viewer display. (int; default: 0) [default=0].
- visir_old_spc_wcal.param.slit_skew¶
Distortion correction: Skew of slit (degrees) (clockwise) (float; default: 0.52) [default=0.52].
- visir_old_spc_wcal.param.spectrum_skew¶
Distortion correction: LMR Skew of spectrum (degrees) (counter- clockwise). Not used in High Resolution (float; default: 1.73) [default=1.73].
- visir_old_spc_wcal.param.vert_arc¶
Distortion correction: LR Detector vertical curvature (pixel). Reduced by a factor 4 in MR. Not used in HR A-side. Increased by a factor 115/52 in HR B-side (float; default: -0.8) [default=-0.8].
- visir_old_spc_wcal.param.hori_arc¶
Distortion correction: LMR Detector horizontal curvature (pixel). Increased by a factor 1.5 in HR A-side. Reduced by a factor 2 in HR B-side (float; default: 0.0) [default=0.0].
- visir_old_spc_wcal.param.rl¶
Reject leftmost columns in spectrum extraction, zero means all columns on the left are used. In cross-dispersion mode a (small) negative number may be used (pixel) (int; default: 0) [default=0].
- visir_old_spc_wcal.param.rr¶
Reject rightmost columns in spectrum extraction, zero means all columns on the right are used. In cross-dispersion mode a (small) negative number may be used (pixel) (int; default: 0) [default=0].
The following code snippet shows the default settings for the available parameters.
import cpl
visir_old_spc_wcal = cpl.Recipe("visir_old_spc_wcal")
visir_old_spc_wcal.param.auto_bpm = True
visir_old_spc_wcal.param.plot = 0
visir_old_spc_wcal.param.slit_skew = 0.52
visir_old_spc_wcal.param.spectrum_skew = 1.73
visir_old_spc_wcal.param.vert_arc = -0.8
visir_old_spc_wcal.param.hori_arc = 0.0
visir_old_spc_wcal.param.rl = 0
visir_old_spc_wcal.param.rr = 0
You may also set or overwrite some or all parameters by the recipe parameter param, as shown in the following example:
import cpl
visir_old_spc_wcal = cpl.Recipe("visir_old_spc_wcal")
[...]
res = visir_old_spc_wcal( ..., param = {"auto_bpm":True, "plot":0})
See also
cpl.Recipe for more information about the recipe object.
Bug reports¶
Please report any problems to Lars Lundin. Alternatively, you may send a report to the ESO User Support Department.
Copyright¶
This file is part of the VISIR Instrument Pipeline Copyright (C) 2004, 2005 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
Code author: Lars Lundin <https://support.eso.org>