Institut für Astronomie und AstrophysikAbteilung AstronomieWaldhäuser Str. 64, D-72076 Tübingen, Germany |
DIST_CIRCLE
Form a square array where each value is its distance to a given center.
Returns a square array in which the value of each element is its distance to a specified center. Useful for circular aperture photometry.
DIST_CIRCLE, IM, N, [ XCEN, YCEN, /DOUBLE ]
N = either a scalar specifying the size of the N x N square output array, or a 2 element vector specifying the size of the N x M rectangular output array.
XCEN,YCEN = Scalars designating the X,Y pixel center. These need not be integers, and need not be located within the output image. If not supplied then the center of the output image is used (XCEN = YCEN = (N-1)/2.).
IM - N by N (or M x N) floating array in which the value of each pixel is equal to its distance to XCEN,YCEN
/DOUBLE - If this keyword is set and nonzero, the output array will be of type DOUBLE rather than floating point.
Total the flux in a circular aperture within 3' of a specified RA and DEC on an 512 x 512 image IM, with a header H. IDL> adxy, H, RA, DEC, x, y ;Convert RA and DEC to X,Y IDL> getrot, H, rot, cdelt ;CDELT gives plate scale deg/pixel IDL> cdelt = cdelt*3600. ;Convert to arc sec/pixel IDL> dist_circle, circle, 512, x, y ;Create a distance circle image IDL> circle = circle*abs(cdelt[0]) ;Distances now given in arcseconds IDL> good = where(circle LT 180) ;Within 3 arc minutes IDL> print,total( IM[good] ) ;Total pixel values within 3'
The speed of DIST_CIRCLE decreases and the the demands on virtual increase as the square of the output dimensions. Users should dimension the output array as small as possible, and re-use the array rather than re-calling DIST_CIRCLE
Adapted from DIST W. Landsman March 1991 Allow a rectangular output array W. Landsman June 1994 Converted to IDL V5.0 W. Landsman September 1997 Add /DOUBLE keyword, make XCEN,YCEN optional W. Landsman Jun 1998
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