% @(#)xcorreimag.hlq 17.1.1.1 (ESO-IPG) 01/25/02 17:44:04 %++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++ %.COPYRIGHT (c) 1990 European Southern Observatory %.IDENT xcorreimag.hlq %.AUTHOR MR,KB, IPG/ESO %.KEYWORDS MIDAS, help files, XCORRELATE/IMAGE %.PURPOSE On-line help file for the command: XCORRELATE/IMAGE %.VERSION 1.0 08-MAY-1989 : Creation, MR,KB %.VERSION 1.1 08-JAN-2002 : Update by H.C.Thomas (MPA, Garching) %---------------------------------------------------------------- \se SECTION./IMAG \es\co XCORRELATE/IMAGE 08-JAN-2002 MR,KB,CT \oc\su XCORRELATE/IMAGE temp spec result shift norm_flag correlate 2 similar 1-dim frames over 2*(shift) bandwith \us\pu Purpose: Correlate 2 similar 1-dim frames over 2*(shift)+1 bandwith. \up\sy Syntax: XCORRELATE/IMAGE temp spec result [shift] [norm_flag] \ys\pa temp = template frame \ap\pa spec = frame to be analyzed \ap\pa result = name of output frame \ap\pa shift = 1/2 bandwith in integer pixels; defaulted to 10 \ap\pa norm_flag = YES or NO for normalizing each pixel of the output frame; defaulted to NO (to be backwards compatible) \ap\sa See also: CONVOLVE/IMAGE, FFT/IMAGE, FFT/FREQUENCY \as\no Note: The template frame should have at least (2*shift)+5 pixels. Identical STEP size (in the first dimension) of the template and analyzed frame is required. If "norm_flag" is set, the 1-dim result frame will contain the correlation coefficient between template and analyzed frame as a function of the shift applied to the latter. It will have (2*shift)+1 pixels and the start will be -shift * stepsize of the analyzed frame. If any input frame is a 2-dim image the first row of that frame is used for the correlation. \on\exs Examples: \ex XCORRELATE/IMAGE anaconda cobra notoca 15 Correlate image `cobra.bdf' with template `anaconda.bdf' over a total of 31 pixels, results are in image `notoca.bdf'. \xe \ex XCORRELATE/IMAGE anaconda cobra notoca 15 yes As above, but the pixels of `notoca.bdf' are normalized. \xe \sxe