The visir_old_img_phot recipe

visir_old_img_phot

Synopsis

Old DRS detector: Sensitivity computation

Description

This recipe computes the conversion factor and the sentitivity of a standard star. It requires a standard star catalog.

The files listed in the Set Of Frames (sof-file) must be tagged: VISIR-std-star-observation.fits IM_CAL_PHOT VISIR-Imaging-Standard-Star-Catalog.fits IMG_STD_CATALOG

The primary product will have a FITS card ‘HIERARCH ESO PRO CATG’ with a string value of ‘IMG_PHOT_COMBINED’

and the corresponding beam-collapsed product will have a FITS card

‘HIERARCH ESO PRO CATG’ with a value of IMG_PHOT_ONEBEAM

Additionally, a bad pixel map with a PRO.CATG of IMG_BPM may be added to the Set Of Frames with tag: BPM.

Constructor

cpl.Recipe("visir_old_img_phot")

Create an object for the recipe visir_old_img_phot.

import cpl
visir_old_img_phot = cpl.Recipe("visir_old_img_phot")

Parameters

visir_old_img_phot.param.nod

An optional ASCII specification of the nodding positions (in case they are missing from the FITS-file). The file must consist of one line per input FITS-file and each line must consist of an integer (which is ignored) followed by a 0 or 1 (to indicate object or sky). (str; default: ‘NONE’) [default=”NONE”].

visir_old_img_phot.param.auto_bpm

Automatic detection and correction of bad pixels (bool; default: True) [default=True].

visir_old_img_phot.param.g

Automatic filtering of glitches (bool; default: False) [default=False].

visir_old_img_phot.param.p

Automatic purging of half-cycle images whose median deviates more than a factor three from the mean of the medians of half-cycle images or whose standard deviation deviates more than a factor three from the mean of their standard deviations (bool; default: False) [default=False].

visir_old_img_phot.param.union

Combine images using their union, as opposed to their intersection (deprecated and ignored, see –combine_method) (bool; default: True) [default=True].

visir_old_img_phot.param.rej

Each resulting pixel is the average of the corresponding (interpolated) pixel value in each jittered image. A positive value, n1, for the first of the two integers specifies that for each pixel the smallest n1 pixel values shall be ignored in the averaging. Similarly, a positive value, n2, for the second of the two integers specifies that for each pixel the largest n2 pixel values shall be ignored in the averaging. (str; default: ‘0-0’) [default=”0-0”].

visir_old_img_phot.param.plot

The recipe can produce a number of predefined plots. Zero means that none of the plots are produced, while increasing values (e.g. 1 or 2) increases the number of plots produced. If the plotting fails a warning is produced, and the recipe continues. The default behaviour of the plotting is to use gnuplot (with option -persist). The recipe currently produces 1D-plots using gnuplot commands. The recipe user can control the actual plotting-command used by the recipe to create the plot by setting the environment variable CPL_PLOTTER. Currently, if CPL_PLOTTER is set it must contain the string ‘gnuplot’. Setting it to ‘cat > my_gnuplot_$$.txt’ causes a number of ASCII-files to be created, which each produce a plot when given as standard input to gnuplot (e.g. later or on a different computer). A finer control of the plotting options can be obtained by writing an executable script, e.g. my_gnuplot.pl, that executes gnuplot after setting the desired gnuplot options (e.g. set terminal pslatex color) and then setting CPL_PLOTTER to my_gnuplot.pl. The predefined plots include plotting of images. Images can be plotted not only with gnuplot, but also using the pnm format. This is controlled with the environment variable CPL_IMAGER. If CPL_IMAGER is set to a string that does not contain the word gnuplot, the recipe will generate the plot in pnm format. E.g. setting CPL_IMAGER to ‘display - &’ will produce a gray-scale image using the image viewer display. (int; default: 0) [default=0].

visir_old_img_phot.param.off

An optional ASCII specification of the offsets in case those in FITS- headers are missing or wrong. The file must consist of one line per input pair of FITS-files, and each line must consist of two numbers which represent the shift in pixels of that image relative to the first image. The first line should thus comprise two zeros. Correct FITS-header offsets mean that the i’th X offset can be gotten from Xoffset_0 - Xoffset_i, where Xoffset_i is the value of ESO SEQ CUMOFFSETX and likewise for Y. (str; default: ‘NONE’) [default=”NONE”].

visir_old_img_phot.param.ref

User-defined refining of the image offsets. See options objs and xcorr (bool; default: False) [default=False].

visir_old_img_phot.param.objs

The shift and add of images needs anchor points that typically are bright objects. These are normally detected automatically but with user-defined refining of offsets enabled, they must be provided by the user through an ASCII file containing one line per anchor point with each line consisting of its x and y coordinate (in pixels). This file is ignored with user-defined refining of offsets disabled. (str; default: ‘NONE’) [default=”NONE”].

visir_old_img_phot.param.xcorr

If user-defined refining of offsets is enabled a cross-correlation of the images is performed. In order to speed up this process, this cross-correlation is performed only on smaller rectangles around the anchor points. The first two parameters is the half-size of this rectangle in pixels. The second pair is the maximum shift in x and y (pixels) evaluated by the cross-correlation on the rectangle. Used only if user-defined refining of offsets is enabled. (str; default: ‘10-10-25-25’) [default=”10-10-25-25”].

visir_old_img_phot.param.jy_val

The flux of the standard star in Jansky (float; default: -999.0) [default=-999.0].

visir_old_img_phot.param.radii

Radii : star_max bg_int bg_ext (str; default: ‘20-20-30’) [default=”20-20-30”].

visir_old_img_phot.param.combine_method

Combine images using one of: 1) Onto the first image (first); 2) Their union (union); 3) Their intersection (inter). NB: Only the ‘first’-method produces an image product with WCS coordinates. A successful ‘first’-method always produces a combined image with dimensions equal to those of the input images. For the ‘union’-method the result image is at least as large as the input images while for the ‘inter’-method the result image is at most as large as the input images (str; default: ‘union’) [default=”union”].

visir_old_img_phot.param.destripe_iterations

Max number of destriping iterations (0 to disable destriping). Horizontal destriping is done first and if no horizontal striping is detected, vertical destriping is performed (int; default: 15) [default=15].

visir_old_img_phot.param.destripe_morpho

Destripe with morphological cleaning (bool; default: False) [default=False].

visir_old_img_phot.param.eccmax

The maximum eccentricity allowed in the combination of the three (in parallel nod/chopping) or four (in perpendicular nod/chopping) beams. In parallel mode, three perfectly aligned points spaced with the chopnod throw will have eccentricity 0, while in perpedicular mode a square with the chopnod throw as the side length will have eccentricity 0 (float; default: 0.25) [default=0.25].

The following code snippet shows the default settings for the available parameters.

import cpl
visir_old_img_phot = cpl.Recipe("visir_old_img_phot")

visir_old_img_phot.param.nod = "NONE"
visir_old_img_phot.param.auto_bpm = True
visir_old_img_phot.param.g = False
visir_old_img_phot.param.p = False
visir_old_img_phot.param.union = True
visir_old_img_phot.param.rej = "0-0"
visir_old_img_phot.param.plot = 0
visir_old_img_phot.param.off = "NONE"
visir_old_img_phot.param.ref = False
visir_old_img_phot.param.objs = "NONE"
visir_old_img_phot.param.xcorr = "10-10-25-25"
visir_old_img_phot.param.jy_val = -999.0
visir_old_img_phot.param.radii = "20-20-30"
visir_old_img_phot.param.combine_method = "union"
visir_old_img_phot.param.destripe_iterations = 15
visir_old_img_phot.param.destripe_morpho = False
visir_old_img_phot.param.eccmax = 0.25

You may also set or overwrite some or all parameters by the recipe parameter param, as shown in the following example:

import cpl
visir_old_img_phot = cpl.Recipe("visir_old_img_phot")
[...]
res = visir_old_img_phot( ..., param = {"nod":"NONE", "auto_bpm":True})

See also

cpl.Recipe for more information about the recipe object.

Bug reports

Please report any problems to Lars Lundin. Alternatively, you may send a report to the ESO User Support Department.