C @(#)cloudpsf.for 17.1.1.1 (ESO-DMD) 01/25/02 17:13:50 C=========================================================================== C Copyright (C) 1995 European Southern Observatory (ESO) C C This program is free software; you can redistribute it and/or C modify it under the terms of the GNU General Public License as C published by the Free Software Foundation; either version 2 of C the License, or (at your option) any later version. C C This program is distributed in the hope that it will be useful, C but WITHOUT ANY WARRANTY; without even the implied warranty of C MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the C GNU General Public License for more details. C C You should have received a copy of the GNU General Public C License along with this program; if not, write to the Free C Software Foundation, Inc., 675 Massachusetts Ave, Cambridge, C MA 02139, USA. C C Correspondence concerning ESO-MIDAS should be addressed as follows: C Internet e-mail: midas@eso.org C Postal address: European Southern Observatory C Data Management Division C Karl-Schwarzschild-Strasse 2 C D 85748 Garching bei Muenchen C GERMANY C=========================================================================== C PROGRAM PSF C************************************************** C M.PIERRE 1-88 C C CALCULATION OF A 1D_GAUSSIAN NORMALIZED C AND CENTERED AT 0 C Modified: START, STEP double precision i/o C C 990805 C************************************************** C IMPLICIT NONE C INTEGER MADRID(1),IMNO INTEGER NCARA,KUN,KNUL,IST,NPIX INTEGER*8 PNTR C REAL START,FNORM REAL FWHM,STEP,DIM(3) C DOUBLE PRECISION DSTA, DSTP C CHARACTER NOMP*60,IDENT*72,CUNIT*80 C COMMON/VMR/MADRID C CALL STSPRO('PSF') C CALL STKRDC('IN_A',1,1,60,NCARA,NOMP,KUN,KNUL,IST) CALL STKRDR('INR',1,1,NCARA,FWHM,KUN,KNUL,IST) CALL STKRDR('CLDDIM',1,3,NCARA,DIM,KUN,KNUL,IST) C STEP =DIM(2) START=-4.*FWHM NPIX =-2.*START/STEP FNORM=.9394373/FWHM*STEP C IDENT='PSF ' CUNIT = ' ' DSTA = START DSTP = STEP CALL STIPUT(NOMP,10,1,1,1,NPIX,DSTA,DSTP,IDENT, : CUNIT,PNTR,IMNO,IST) CALL IMAGE(MADRID(PNTR),NPIX,STEP,START,FWHM,FNORM) CALL STSEPI END C SUBROUTINE IMAGE(Y,NPIX,STEP,START,FWHM,FNORM) INTEGER NPIX,I REAL Y(1),START,STEP,FWHM,FNORM,WL DO 10 I=1,NPIX WL=START+FLOAT(I-1)*STEP Y(I)=FNORM*EXP(-0.69315*((2.*WL/FWHM)**2)) 10 CONTINUE RETURN END C