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author | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
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committer | Joe Hunkeler <jhunkeler@gmail.com> | 2015-08-11 16:51:37 -0400 |
commit | 40e5a5811c6ffce9b0974e93cdd927cbcf60c157 (patch) | |
tree | 4464880c571602d54f6ae114729bf62a89518057 /pkg/images/immatch/doc/imcentroid.hlp | |
download | iraf-osx-40e5a5811c6ffce9b0974e93cdd927cbcf60c157.tar.gz |
Repatch (from linux) of OSX IRAF
Diffstat (limited to 'pkg/images/immatch/doc/imcentroid.hlp')
-rw-r--r-- | pkg/images/immatch/doc/imcentroid.hlp | 257 |
1 files changed, 257 insertions, 0 deletions
diff --git a/pkg/images/immatch/doc/imcentroid.hlp b/pkg/images/immatch/doc/imcentroid.hlp new file mode 100644 index 00000000..c284d9be --- /dev/null +++ b/pkg/images/immatch/doc/imcentroid.hlp @@ -0,0 +1,257 @@ +.help imcentroid Jan97 images.immatch +.ih +NAME +imcentroid -- center sources in images, optionally find shifts + +.ih +USAGE +imcentroid input reference coords + +.ih +PARAMETERS + +.ls input +The list of images within which sources are to be centered. If a +\fIreference\fR image is specified, imcentroid will calculate the mean +X and Y shifts between the centered sources within each image and those +same sources within the reference image. The input image list +should normally include the reference image so that its borders are +used in the calculation of the overlap region. +.le +.ls reference = "" +The reference image to which the input images will be aligned. If +a reference image is specified the mean X and Y shifts between each of +the input images and the reference image will be calculated, otherwise +only the centers for the individual sources will be reported. +.le +.ls coords +A text file containing the coordinates of the registration objects to +be centered in each image, one object per line with the x and y +coordinates in columns one and two respectively. These coordinates +should be measured in the frame of the reference image. +.le +.ls shifts = "" +A text file containing the initial estimate for each image of the +shift in each axis relative to the reference image. These +estimates are used to modify the coordinates of the registration +objects prior to centering. The format of the file is one image per +line with the fractional x and y shifts in columns one and two +respectively. The sense of the shifts is such that: +Xshift =Xref - Xin and shift= Yref - Yin. If shifts is undefined, +a coarse centering pass will be made to attempt to determine +the initial shifts. +.le +.ls boxsize = 7 +The size in pixels of the box to use for the final centering, during +which all the sources in the coords file are recentered in each image +using the initial estimate of the relative shift for each image. +Care should be taken to choose an appropriate value for this parameter, +since it is highly data dependent. +.le +.ls bigbox = 11 +The size in pixels of the box to use for coarse centering. The coarse +pass through the centering algorithm is made with the box centered at +the nominal position of the first source in the coordinate list. +Coarse centering is performed only if the shifts file is undefined. +Care should be taken to choose an appropriate value for this parameter, +since it is highly data dependent. Large value should be suspect until +the final results are checked to see that the centering did not converge +on the wrong coordinates, although the usual result for an inappropriate +bigbox size is that the algorithm fails to converge and the task +aborts. +.le +.ls negative = no +Are the features negative ? +.le +.ls background = INDEF +The absolute reference level for the marginal centroid calculation. +If background is INDEF, this is set to the mean value (between the +thresholds) of the individual sources. +.le +.ls lower = INDEF +The lower threshold for the data. Individual pixels less than this +value will be given zero weight in the centroids. +.le +.ls upper = INDEF +The upper threshold for the data. Individual pixels greater than this +value will be given zero weight in the centroids. +.le +.ls niterate = 3 +The maximum number of centering iterations to perform. The centering +will halt when this limit is reached or when the desired tolerance +is achieved. +.le +.ls tolerance = 0 +The tolerance for convergence of the centering algorithm. This is the +integral shift of the centering box from one iteration to the next. +.le +.ls maxshift = INDEFR +The maximum permitted difference between the predicted shift and the +the computed shift for each object. Objects with shifts greater than +maxshift are ignored. If maxshift is undefined no shift checking is done. +.le +.ls verbose = yes +Print the centers for the individual objects ? If verbose is no +only the shifts relative to the reference coordinates will be reported. +If no reference image is supplied, verbose is automatically set to yes. +.le + +.ih +DESCRIPTION + +IMCENTROID measures the X and Y coordinates of a list of sources in a +list of images and finds the mean X and Y shifts between the input +images \fIinput\fR and a \fIreference\fR image, where the shifts are +defined as the shifts that should be added to the input image coordinates to +convert them into the reference coordinates. The task is meant to +address the class of two dimensional image registration problems in +which the images have the same pixel scale, are shifted relative to +each other by simple translations in each axis, and contain enough high +signal-to-noise, pointlike sources in common to form good average +positions. The basic operation of the task is to find centers for the +list of registration objects in the coordinate frame of each image and +then to subtract the corresponding centers found in the reference +image. The shifts of the objects are averaged for each image. + +A list of the X and Y coordinates of the registration objects should be +provided in the coordinates file \fIcoords\fR. The registration objects do not +all have to be common to each frame, rather only that subset of the +objects that is contained within the bounds of a given image will be +centered. Only the objects that are common to both the given image and +the reference will be used to calculate the shifts. The coordinates +should be measured in the frame of the reference image\fIreference\fR. +If coarse centering is to be done, which is to say, if no \fIshifts\fR file is +provided, then the first registration source should be separated from +other sources by at least the maximum expected relative shift. + +An initial estimate of the shifts between each of the input images +\fIinput\fR and the reference image \fIreference\fR is required for the +centering algorithm (a marginal centroid) to work. This estimate can be +explicitly supplied in the text file \fIshifts\fR where Xshift = Xref -Xin +and Yshift = Yref -Y in, or can be generated from the images by measuring +the relative shift of the first source listed in the coordinates file +\fIcoords\fR for each input image. This coarse +centering pass requires that the first source be detached from other +sources and from the border of each image by a distance that is at +least the maximum shift between the reference and input image. This +source should be pointlike and have a high signal to noise ratio. The +value of the \fIbigbox\fR parameter should be chosen to include the +location of the source in each of the images to be aligned while +excluding other sources. Large values of \fIbigbox\fR should be held +suspect until the final convergence of the centering algorithm is +verified, although given a small value for the \fItolerance\fR, the +quality of the final centers is independent of the estimate for the +initial shifts. Better convergence may also be obtained by increasing +the \fIniterate\fR parameter, although the default value of three +should work for most cases. \fINiterate\fR should be kept small to +avoid runaway. + +The \fIboxsize\fR parameter controls the size of the centering box for +the fine centering pass and should be chosen so as to exclude sky +background and other sources while including the wings of the point +spread function. The sense of the shifts that are calculated is +consistent with the file supplied to the \fIshifts\fR parameter and +with that used with the IMSHIFT task. + +IMCENTROID may be used with a set of input images which vary in size. +This can result in vignetting of the calculated overlap region because +of the nature of tasks such as IMSHIFT to preserve the size of an input +image. To visualize this, imagine a large reference image and a single +small image to be aligned to it, both containing the same registration +object which is at the center of each image. IMCENTROID will cause the +coordinate system of the small image to be shifted such that the object +will be positioned at the same pixel location as in the reference. If +the shift is performed, a large fraction of the area of the small image +may be shifted outside of its own borders, whereas the physical overlap +of the large and small images includes ALL of the pixels of the small +image. In the case of such vignetting, IMCENTROID will print a warning +message and both the vignetted and unvignetted trim sections. Note +that the vignetting will not occur if the small image is used as the +reference image. + +The vignetting message may also be printed if the input images are all +the same size but the reference image is not included in the list. +This will occur if the sense of the measured shifts in a coordinate are +all positive or all negative since in this case the border of the +reference image would have provided one of the limits to the trim +section. The reality of this vignetting depends on your point of view. + +Note that many of these difficulties are due to the intrinsically fuzzy +nature of the process of image registration. This all leads to a few +guidelines: + +.nf + o Include the reference image in the input image list + + o Use the smallest image as the reference image + + o Choose the reference image such that the input images + are scattered to either side in the shifts in each axis + + o Align images that are the same size, OR + + o Pad dissimilar sized images with blanks to the largest size +.fi + +.ih +CENTERING ALGORITHM + +The algorithm is a "marginal" centroid in which the fit for each axis +is performed separately upon a vector created by collapsing the +centering box perpendicular to that axis. The centroid is calculated +with respect to the level specified by \fIbackground\fR. If +\fIbackground\fR is INDEF, the reference level for each source in each +image is the local mean for those pixels that lie between the +\fIlower\fR and \fIupper\fR thresholds. The thresholds are set to the +local data minimum or maximum if \fIlower\fR or \fIupper\fR, +respectively, are INDEF. If \fInegative\fR is yes, than the marginal +vector will be inverted before being passed to the centroid algorithm. + +The maximum number of centering iterations and the tolerance for +convergence are controlled by \fIniterate\fR and \fItolerance\fR. Note +that the tolerance is an integer value that represents the maximum +movement of the centering box between two successive iterations. The +default value of 0 requires that the centroid lie within the center +pixel of the centering box which is \fIboxsize\fR in extent (note that +\fIboxsize\fR must be an odd number). This should normally be the case +for bright, circularly symmetric point sources in images with a flat +sky background. If the registration sources are not circular symmetric +try increasing the tolerance gingerly. If the sky background is not +flat, but varies across the image, it can be removed before processing. + +.ih +EXAMPLES + +1. Calculate the shifts between three images using the first image +as a reference image and the list of registration star coordinates in +the file "x1.coords". + +.nf + cl> imcentroid x1,x2,x3 x1 x1.coords +.fi + +2. Calculate the shifts between a list of images contained in the file +"imlist": + +.nf + pr> imcentroid @imlist x1 x1.coords +.fi + +3. Perform the centering, but don't calculate the shifts, i.e., don't +supply a reference image. Note that the \fIinput\fR list of shifts, +or a coarse centering pass are still needed: + +.nf + pr> imcentroid @imlist "" x1.coords +.fi + +.ih +BUGS +The coarse centering portion of the algorithm can be fooled if the +first source on the list is not well separated from other sources, or +if the first source has a low signal to noise ratio, or if there is a +complicated shape to the background. +.ih +SEE ALSO +imalign, imshift, xregister, geomap, geotran +.endhelp |