The kmos_dark recipe =============================================================== .. data:: kmos_dark Synopsis -------- Create master dark frame & bad pixel mask Description ----------- This recipe calculates the master dark frame. It is recommended to provide three or more dark exposures to produce a reasonable master with associated noise. Input files ^^^^^^^^^^^^ :: DO CATG Type Explanation Required #Frames ------- ----- ----------- -------- ------- DARK RAW Dark exposures Y 1-n (at least 3 frames recommended) Output files ^^^^^^^^^^^^ :: DO CATG Type Explanation ------- ----- ----------- MASTER_DARK F2D Calculated master dark frames BADPIXEL_DARK B2D Associated badpixel frames Constructor ----------- .. method:: cpl.Recipe("kmos_dark") :noindex: Create an object for the recipe kmos_dark. :: import cpl kmos_dark = cpl.Recipe("kmos_dark") Parameters ---------- .. py:attribute:: kmos_dark.param.oscan Apply Overscan Correction (bool; default: True) [default=True]. .. py:attribute:: kmos_dark.param.pos_bad_pix_rej The positive rejection threshold for bad pixels (float; default: 50.0) [default=50.0]. .. py:attribute:: kmos_dark.param.neg_bad_pix_rej The negative rejection threshold for bad pixels (float; default: 50.0) [default=50.0]. .. py:attribute:: kmos_dark.param.file_extension Controls if EXPTIME should be appended to product filenames (bool; default: False) [default=False]. .. py:attribute:: kmos_dark.param.cmethod Apply "average", "median", "sum", "min_max." or "ksigma". (str; default: 'ksigma') [default="ksigma"]. .. py:attribute:: kmos_dark.param.cpos_rej The positive rejection threshold for kappa-sigma-clipping (sigma). (float; default: 3.0) [default=3.0]. .. py:attribute:: kmos_dark.param.cneg_rej The negative rejection threshold for kappa-sigma-clipping (sigma). (float; default: 3.0) [default=3.0]. .. py:attribute:: kmos_dark.param.citer The number of iterations for kappa-sigma-clipping. (int; default: 3) [default=3]. .. py:attribute:: kmos_dark.param.cmax The number of maximum pixel values to clip with min/max-clipping. (int; default: 1) [default=1]. .. py:attribute:: kmos_dark.param.cmin The number of minimum pixel values to clip with min/max-clipping. (int; default: 1) [default=1]. The following code snippet shows the default settings for the available parameters. :: import cpl kmos_dark = cpl.Recipe("kmos_dark") kmos_dark.param.oscan = True kmos_dark.param.pos_bad_pix_rej = 50.0 kmos_dark.param.neg_bad_pix_rej = 50.0 kmos_dark.param.file_extension = False kmos_dark.param.cmethod = "ksigma" kmos_dark.param.cpos_rej = 3.0 kmos_dark.param.cneg_rej = 3.0 kmos_dark.param.citer = 3 kmos_dark.param.cmax = 1 kmos_dark.param.cmin = 1 You may also set or overwrite some or all parameters by the recipe parameter `param`, as shown in the following example: :: import cpl kmos_dark = cpl.Recipe("kmos_dark") [...] res = kmos_dark( ..., param = {"oscan":True, "pos_bad_pix_rej":50.0}) .. seealso:: `cpl.Recipe `_ for more information about the recipe object. Bug reports ----------- Please report any problems to `Alex Agudo Berbel, Yves Jung `_. Alternatively, you may send a report to the `ESO User Support Department `_. Copyright --------- This file is part of the CRIRES Instrument Pipeline Copyright (C) 2002,2003 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 .. codeauthor:: Alex Agudo Berbel, Yves Jung