The fors_extract_slits recipe¶
-
fors_extract_slits
¶
Synopsis¶
Spatial rectification of spectral image
Description¶
This recipe is used to extract MOS/MXU slit spectra, following their curvature, and to remap them into a spatially rectified image.
Please refer to the FORS Pipeline User’s Manual for details about the spectra remapping technique. Note however that the interpolation is done exclusively along the spatial direction, and therefore the output rectified image will have the same x size of the input spectral image.
In the table below the MXU acronym can be alternatively read as MOS.
Input files¶
DO category: Type: Explanation: Required:
LAMP_UNBIAS_MXU
or SCIENCE_UNBIAS_MXU
or SCIENCE_UNFLAT_MXU
or STANDARD_UNBIAS_MXU
or STANDARD_UNFLAT_MXU
or UNMAPPED_SCI_MXU
or UNMAPPED_STD_MXU
or UNMAPPED_SKY_SCI_MXU
or UNMAPPED_SKY_STD_MXU Calib Spectral frame Y
SLIT_LOCATION_DETECT_MXU
or SLIT_LOCATION_MXU Calib Master flat frame Y
CURV_COEFF_MXU Calib Spectral curvature Y
GRISM_TABLE Calib Grism table .
Output files¶
DO category: Data type: Explanation:
RECTIFIED_LAMP_MXU
or RECTIFIED_ALL_SCI_MXU
or RECTIFIED_ALL_STD_MXU
or RECTIFIED_SCI_MXU
or RECTIFIED_STD_MXU
or RECTIFIED_SKY_SCI_MXU
or RECTIFIED_SKY_STD_MXU FITS image Rectified slit spectra
Constructor¶
-
cpl.
Recipe
("fors_extract_slits") Create an object for the recipe fors_extract_slits.
import cpl
fors_extract_slits = cpl.Recipe("fors_extract_slits")
Parameters¶
-
fors_extract_slits.param.
dispersion
¶ Expected spectral dispersion (Angstrom/pixel) (float; default: 0.0) [default=0.0].
-
fors_extract_slits.param.
startwavelength
¶ Start wavelength in spectral extraction (float; default: 0.0) [default=0.0].
-
fors_extract_slits.param.
endwavelength
¶ End wavelength in spectral extraction (float; default: 0.0) [default=0.0].
-
fors_extract_slits.param.
flux
¶ Apply flux conservation (bool; default: True) [default=True].
The following code snippet shows the default settings for the available parameters.
import cpl
fors_extract_slits = cpl.Recipe("fors_extract_slits")
fors_extract_slits.param.dispersion = 0.0
fors_extract_slits.param.startwavelength = 0.0
fors_extract_slits.param.endwavelength = 0.0
fors_extract_slits.param.flux = True
You may also set or overwrite some or all parameters by the recipe parameter param, as shown in the following example:
import cpl
fors_extract_slits = cpl.Recipe("fors_extract_slits")
[...]
res = fors_extract_slits( ..., param = {"dispersion":0.0, "startwavelength":0.0})
See also
cpl.Recipe for more information about the recipe object.
Bug reports¶
Please report any problems to Carlo Izzo. Alternatively, you may send a report to the ESO User Support Department.
Copyright¶
This file is currently part of the FORS Instrument Pipeline Copyright (C) 2002-2010 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 02110-1301 USA
Code author: Carlo Izzo <usd-help@eso.org>