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diff --git a/pkg/proto/doc/imcntr.hlp b/pkg/proto/doc/imcntr.hlp new file mode 100644 index 00000000..b715fefd --- /dev/null +++ b/pkg/proto/doc/imcntr.hlp @@ -0,0 +1,61 @@ +.help imcntr Dec85 proto +.ih +NAME +imcntr -- locate the center of a stellar image +.ih +USAGE +imcntr input x_init y_init +.ih +PARAMETERS +.ls input +The list of images which contain the star to be centered. +.le +.ls x_init +The approximate column coordinate as a starting point for the centering. +.le +.ls y_init +The approximate line (row) coordinate as a starting point for the centering. +.le +.ls cboxsize = 5 +The size of the extraction box to be used during the centering process. +.le +.ih +DESCRIPTION +Given the approximate coordinates of the center of an object, (x_init, y_init), +IMCNTR will compute a more accurate center using the algorithms described in +the Kitt Peak publication "Stellar Magnitudes from Digital Images" under +the Mountain Photometry Code section. Briefly, this algorithm computes +the sum of all the rows and the sum of all the columns in the extraction +box. These are called "marginal distributions". The center in x (column +value) is then the center of gravity of the row marginal, and the center +in y is the center of gravity of the column marginal. +If the resultant x or y center value deviates from the original input +approximate starting points by more than 1 pixel, the process is repeated +once more around the new center. Only one iteration is attempted to +avoid runaway if a bright star is nearby. + +Because the centers are computed independently for x and y, the result +may be considered inferior to a true two-dimensional centering algorithm. +Nevertheless, in practice the results appear to be very usable. + +The value for the box size should be an odd value. If chosen too large, +nearby objects will affect the result. If too small, the center will be +poorly defined. +.ih +EXAMPLES +1. The following example locates the center of a star near (123, 234) +in 3 images. +.sp 1 +.nj +.nf +cl> imcntr m92red,m92blu,m92grn 123 234 +.fi +.ju +.ih +BUGS +The routine will probably fail if the desired object is within 2 or 3 pixels +of the image boundary. +.ih +SEE ALSO +pradprof +.endhelp |