The fors_resample recipe¶
-
fors_resample
¶
Synopsis¶
Resample input spectra at constant wavelength step
Description¶
This recipe is used to resample at constant wavelength step spatially rectified spectra. The input frames are produced using either the recipe fors_extract_slits in the case of MOS/MXU multi slit exposures, or the recipes fors_remove_bias and fors_flatfield in the case of LSS or long-slit like MOS/MXU data. Only in case of LSS or LSS-like data the SLIT_LOCATION table is required in input. Please refer to the FORS Pipeline User’s Manual for more details.
In the table below the MXU acronym can also be read as MOS and LSS, SCI can be read as STD, and SCIENCE as STANDARD.
Input files¶
DO category: Type: Explanation: Required:
LAMP_UNBIAS_MXU
or SCIENCE_UNBIAS_MXU
or SCIENCE_UNFLAT_MXU
or RECTIFIED_LAMP_MXU
or RECTIFIED_ALL_SCI_MXU
or RECTIFIED_SCI_MXU
or RECTIFIED_SKY_SCI_MXU Calib Frame to resample Y
DISP_COEFF_MXU
or DISP_COEFF_SCI_MXU Calib Dispersion coefficients Y
SLIT_LOCATION_MXU Calib Slit location table Y
GRISM_TABLE Calib Grism table .
Output files¶
DO category: Data type: Explanation:
MAPPED_LAMP_MXU
or MAPPED_ALL_SCI_MXU
or MAPPED_SCI_MXU
or MAPPED_SKY_SCI_MXU FITS image Resampled spectra
Constructor¶
-
cpl.
Recipe
("fors_resample") Create an object for the recipe fors_resample.
import cpl
fors_resample = cpl.Recipe("fors_resample")
Parameters¶
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fors_resample.param.
dispersion
¶ Expected spectral dispersion (Angstrom/pixel) (float; default: 0.0) [default=0.0].
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fors_resample.param.
startwavelength
¶ Start wavelength in spectral extraction (float; default: 0.0) [default=0.0].
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fors_resample.param.
endwavelength
¶ End wavelength in spectral extraction (float; default: 0.0) [default=0.0].
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fors_resample.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_resample = cpl.Recipe("fors_resample")
fors_resample.param.dispersion = 0.0
fors_resample.param.startwavelength = 0.0
fors_resample.param.endwavelength = 0.0
fors_resample.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_resample = cpl.Recipe("fors_resample")
[...]
res = fors_resample( ..., 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>