The vmifucalib recipe¶
- vmifucalib¶
Synopsis¶
Generate IFU calibrations from a set of flat and arc lamp exposures.
Description¶
This recipe produces the extraction mask, the wavelength calibration, and the relative transmission correction, from a set of flat field and one arc lamp exposures (IFU mode).
Input files¶
DO category: Type: Explanation: Required:
IFU_SCREEN_FLAT Raw Flat field Y
IFU_ARC_SPECTRUM Raw Arc spectrum .
LINE_CATALOG Calib Arc line catalog .
MASTER_BIAS Calib Master bias Y
IFU_IDENT Calib Fiber identification .
CCD_TABLE Calib Bad pixel table .
Output files¶
DO category: Data type: Explanation:
IFU_MASTER_SCREEN_FLAT FITS image Stack of all raw flat fields
IFU_ARC_SPECTRUM_EXTRACTED FITS image Extracted arc spectra
IFU_FLAT_SPECTRUM_EXTRACTED FITS image Extracted flat field spectra
IFU_TRACE FITS table Extraction mask
IFU_IDS FITS table Wavelength calibration
IFU_TRANSMISSION FITS table Transmission correction
An arc spectrum exposure may not be specified in input, but in that case no wavelength calibration nor fiber relative transmission correction will be computed, and further reduction of associated scientific data will not be possible; the only products in this case will be the stack of all the input raw flat field exposures, and the extraction mask. If the arc spectrum exposure is specified in input, then also a line catalog must be given. The fiber identification table, if given, ensures that all spectra will be safely identified and assigned to the correct spatial position, but in most cases it will be possible to reduce the data even without specifying this table in the input SOF. A CCD table must be specified only if a bad pixel cleaning is requested.
For more details, please refer to the VIMOS Pipeline User’s Guide.
Constructor¶
- cpl.Recipe("vmifucalib")
Create an object for the recipe vmifucalib.
import cpl
vmifucalib = cpl.Recipe("vmifucalib")
Parameters¶
- vmifucalib.param.AllowSingleFrames¶
Flat fields combination method is ignored. (bool; default: True) [default=True].
- vmifucalib.param.StackMethod¶
Flat fields combination method. (str; default: ‘MinMax’) [default=”MinMax”].
- vmifucalib.param.KSigmaLow¶
Low threshold for K-sigma clipping method. (float; default: 5.0) [default=5.0].
- vmifucalib.param.KSigmaHigh¶
High threshold for K-sigma clipping method. (float; default: 5.0) [default=5.0].
- vmifucalib.param.MinRejection¶
Number of lowest rejected values for rejection method. (int; default: 0) [default=0].
- vmifucalib.param.MaxRejection¶
Number of highest rejected values for rejection method. (int; default: 1) [default=1].
- vmifucalib.param.BiasMethod¶
Bias removal method. (str; default: ‘Zmaster’) [default=”Zmaster”].
- vmifucalib.param.CleanBadPixel¶
Bad pixel correction on master flat field. (bool; default: False) [default=False].
- vmifucalib.param.ApplyTransmission¶
Apply transmission correction to extracted arc lamp spectra (bool; default: True) [default=True].
- vmifucalib.param.MaxIdsRms¶
Maximum tolerated RMS of residuals in IDS fit (float; default: 2.0) [default=2.0].
- vmifucalib.param.LineIdent¶
Arc line identification method. (str; default: ‘Blind’) [default=”Blind”].
- vmifucalib.param.MaxTraceRejection¶
Maximum percentage of rejected positions in fiber spectra tracing (int; default: 33) [default=33].
- vmifucalib.param.ComputeQC¶
Compute QC1 parameters (bool; default: True) [default=True].
The following code snippet shows the default settings for the available parameters.
import cpl
vmifucalib = cpl.Recipe("vmifucalib")
vmifucalib.param.AllowSingleFrames = True
vmifucalib.param.StackMethod = "MinMax"
vmifucalib.param.KSigmaLow = 5.0
vmifucalib.param.KSigmaHigh = 5.0
vmifucalib.param.MinRejection = 0
vmifucalib.param.MaxRejection = 1
vmifucalib.param.BiasMethod = "Zmaster"
vmifucalib.param.CleanBadPixel = False
vmifucalib.param.ApplyTransmission = True
vmifucalib.param.MaxIdsRms = 2.0
vmifucalib.param.LineIdent = "Blind"
vmifucalib.param.MaxTraceRejection = 33
vmifucalib.param.ComputeQC = True
You may also set or overwrite some or all parameters by the recipe parameter param, as shown in the following example:
import cpl
vmifucalib = cpl.Recipe("vmifucalib")
[...]
res = vmifucalib( ..., param = {"AllowSingleFrames":True, "StackMethod":"MinMax"})
See also
cpl.Recipe for more information about the recipe object.
Bug reports¶
Please report any problems to ESO VIMOS Pipeline Team and VIMOS Consortium. Alternatively, you may send a report to the ESO User Support Department.
Copyright¶
This file is part of the VIMOS Instrument Pipeline Copyright (C) 2019 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
Code author: ESO VIMOS Pipeline Team and VIMOS Consortium <https://support.eso.org>