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Institut für Astronomie und Astrophysik

Abteilung Astronomie

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DAOERF Source code in daoerf.pro

DAOERF

Name
       DAOERF
Purpose
       Calulates the intensity, and derivatives, of a 2-d Gaussian PSF
Explanation
       Corrects for the finite size of a pixel by integrating the Gaussian
       over the size of the pixel.    Used in the IDL-DAOPHOT sequence.
Calling Sequence
       DAOERF, XIN, YIN, A, F, [ PDER ]
Input Parameters
       XIN - input scalar, vector or array, giving X coordinate values
       YIN - input scalar, vector or array, giving Y coordinate values, must
               have same number of elements as XIN.
       A - 5 element parameter array describing the Gaussian
               A(0) - peak intensity
               A(1) - X position of peak intensity (centroid)
               A(2) - Y position of peak intensity (centroid)
               A(3) - X sigma of the gaussian (=FWHM/2.345)
               A(4) - Y sigma of gaussian
Output Parameters
       F - array containing value of the function at each (XIN,YIN)
           The number of output elements in F and PDER is identical with
               the number of elements in X and Y
Optional Output
       PDER - 2 dimensional array of size (NPTS,5) giving the analytic
               derivative at each value of F with respect to each parameter A.
Revision History
       Written: W. Landsman                October, 1987
       Converted to IDL V5.0   W. Landsman   September 1997

Last modified by pro2html on 2001 April 26 at 03:13 UTC

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Jörn Wilms (wilms@astro.uni-tuebingen.de)
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