The fors_img_screen_flat recipe¶
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fors_img_screen_flat
¶
Synopsis¶
Compute master screen flat frame
Description¶
After bias subtraction, the input flat field frames are combined using the given stack method. The combined frame is finally normalised dividing it by its large scale illumination trend. The large scale trend is obtained by applying a median filter with a large kernel. To avoid boundary effects, the median filter is applied only to the specified region.
The overscan regions, if present, are removed from the result.
Input files¶
DO category: Type: Explanation: Required:
SCREEN_FLAT_IMG Raw Screen flat field Y
MASTER_BIAS Raw Master bias Y
Output files¶
DO category: Data type: Explanation:
MASTER_SCREEN_FLAT_IMG FITS image Master screen flat field
Constructor¶
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cpl.
Recipe
("fors_img_screen_flat") Create an object for the recipe fors_img_screen_flat.
import cpl
fors_img_screen_flat = cpl.Recipe("fors_img_screen_flat")
Parameters¶
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fors_img_screen_flat.param.
stack_method
¶ Frames combination method (str; default: ‘average’) [default=”average”].
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fors_img_screen_flat.param.
minrejection
¶ Number of lowest values to be rejected (int; default: 1) [default=1].
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fors_img_screen_flat.param.
maxrejection
¶ Number of highest values to be rejected (int; default: 1) [default=1].
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fors_img_screen_flat.param.
klow
¶ Low threshold in ksigma method (float; default: 3.0) [default=3.0].
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fors_img_screen_flat.param.
khigh
¶ High threshold in ksigma method (float; default: 3.0) [default=3.0].
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fors_img_screen_flat.param.
kiter
¶ Max number of iterations in ksigma method (int; default: 999) [default=999].
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fors_img_screen_flat.param.
xradius
¶ Median filter x radius (unbinned pixels) (int; default: 50) [default=50].
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fors_img_screen_flat.param.
yradius
¶ Median filter y radius (unbinned pixels) (int; default: 50) [default=50].
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fors_img_screen_flat.param.
degree
¶ Degree of fitting polynomial (int; default: -1) [default=-1].
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fors_img_screen_flat.param.
sampling
¶ Sampling interval for fitting (int; default: 100) [default=100].
The following code snippet shows the default settings for the available parameters.
import cpl
fors_img_screen_flat = cpl.Recipe("fors_img_screen_flat")
fors_img_screen_flat.param.stack_method = "average"
fors_img_screen_flat.param.minrejection = 1
fors_img_screen_flat.param.maxrejection = 1
fors_img_screen_flat.param.klow = 3.0
fors_img_screen_flat.param.khigh = 3.0
fors_img_screen_flat.param.kiter = 999
fors_img_screen_flat.param.xradius = 50
fors_img_screen_flat.param.yradius = 50
fors_img_screen_flat.param.degree = -1
fors_img_screen_flat.param.sampling = 100
You may also set or overwrite some or all parameters by the recipe parameter param, as shown in the following example:
import cpl
fors_img_screen_flat = cpl.Recipe("fors_img_screen_flat")
[...]
res = fors_img_screen_flat( ..., param = {"stack_method":"average", "minrejection":1})
See also
cpl.Recipe for more information about the recipe object.
Bug reports¶
Please report any problems to Jonas M. Larsen. 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) 2002-2011 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: Jonas M. Larsen <usd-help@eso.org>