pro hboxave, oldim, oldhd, newim, newhd, box, ERRMSG = errmsg ;Boxaverage and update header ;+ ; NAME: ; HBOXAVE ; PURPOSE: ; Box average an image array and update the FITS header array ; EXPLANATION: ; The function BOXAVE() is used. This procedure is recommended for ; integer images when photometric precision is desired, because it ; performs intermediate steps using REAL*4 arithmetic. Otherwise, the ; procedure HREBIN is much faster. ; ; CALLING SEQUENCE: ; HBOXAVE, Oldim, Oldhd, Newim, Hewhd, box ; or ; HBOXAVE, Oldim, Oldhd, box ; ; INPUTS: ; Oldim - the original image array ; Oldhd - the original image FITS header, string array ; ; OPTIONAL INPUTS: ; box - the box size to be used, integer scalar. If omitted, then ; HBOXAVE will prompt for this parameter. ; ; OPTIONAL OUTPUTS: ; Newim - the image after boxaveraging ; Newhd - header for newim containing updated astrometry info ; If output parameters are not supplied, the program ; will modify the input parameters OLDIM and OLDHD ; to contain the new array and updated header. ; OPTIONAL KEYWORD OUTPUT: ; ERRMSG - If this keyword is supplied, then any error mesasges will be ; returned to the user in this parameter rather than depending on ; on the MESSAGE routine in IDL. If no errors are encountered ; then a null string is returned. ; ; PROCEDURE: ; The parameters BSCALE, NAXIS1, NAXIS2, CRPIX1, and CRPIX2 and ; the CD (or CDELT) parameters are updated for the new FITS header. ; ; EXAMPLE: ; Compress the image in a FITS file 'image.fits' by a factor of 4 and ; update the astrometry in the FITS header ; ; IDL> im = readfits('image.fits',hdr) ;Read FITS file into IDL arrays ; IDL> hboxave, im, hdr, 4 ;Boxaverage by 4 ; IDL> writefits,'image.fits',im,hdr ;Write a new FITS file ; ; CALLED PROCEDURES: ; CHECK_FITS - Check that the FITS header is appropriate to the image ; BOXAVE() - Performs box averaging of an image ; SXPAR(), SXADDPAR - Read and write FITS keyword values ; ; MODIFICATION HISTORY: ; Written, Aug. 1986 W. Landsman, STI Corp. ; IDLV2 changes, sxaddpar format keyword added, J. Isensee, July,1990 ; Fix 0.5 pixel offset in new CRPIX computation W. Landsman, Dec, 1991 ; Update BSCALE even if no astrometry present W. Landsman, May 1997 ; Converted to IDL V5.0 W. Landsman September 1997 ; Added ERRMSG keyword, Use double formatting W. Landsman April 2000 ; Recognize PC matrix astrometry format W. Landsman December 2001 ;- On_error,2 ;Return to caller on error npar = N_params() if ( npar LT 2 ) then begin ;Check # of parameters print,'Syntax: HBOXAVE, oldim, oldhd, [ newim, newhd, box, ERRMSG = ]' print,' or HBOXAVE, oldim, oldhd, [ box, ERRMSG = ]' return endif save_err = arg_present(errmsg) ;Does user want to return error messages? ; Check for valid 2-D image & header check_FITS, oldim, oldhd, dimen, /NOTYPE, ERRMSG = errmsg if errmsg NE '' then begin if not save_err then message,'ERROR - ' + errmsg,/CON return endif if N_elements(dimen) NE 2 then begin errmsg = 'Input image array must be 2-dimensional' if not save_err then message,'ERROR - ' + errmsg,/CON return endif xsize = dimen[0] & ysize = dimen[1] if npar EQ 3 then begin box = newim endif else if (npar NE 5) then begin ;prompt for box size print,'Boxaverage an image and update header' print,'Original array size is '+ strn(xsize) + ' by ' + strn(ysize) read, 'Enter width of box to be used in box average: ',box endif box = fix(box) ;Check for integer type if N_elements(box) NE 1 then begin box = 0 read, 'Enter width of box to be used in box average: ',box endif newx = xsize/float(box) newy = ysize/float(box) if (newx*box NE xsize) or (newy*box NE ysize) then $ message,'ERROR - Box size does not evenly divide image size' if npar GT 3 then newim = boxave( oldim, box) else $ oldim = boxave( oldim, box) newhd = oldhd sxaddpar, newhd, 'NAXIS1', fix(newx) sxaddpar, newhd, 'NAXIS2', fix(newy) label = 'HBOXAVE:' + strmid( systime(), 4, 20) sxaddpar, newhd, 'HISTORY', label + ' Original Image Size Was ' + $ strn(xsize) + ' by ' + strn(ysize) sxaddpar, newhd, 'HISTORY',label+' Box Width: '+ strn(box)+' Pixels' ; Update astrometry info if it exists extast, oldhd, astr, noparams if noparams GE 0 then begin pix_ratio = box*box ;Ratio of old to new pixel areas crpix = (astr.crpix - 0.5)/box + 0.5 sxaddpar, newhd, 'CRPIX1', crpix[0] sxaddpar, newhd, 'CRPIX2', crpix[1] if (noparams NE 2) then begin cdelt = astr.cdelt sxaddpar, newhd, 'CDELT1', CDELT[0]*box sxaddpar, newhd, 'CDELT2', CDELT[1]*box endif else begin ;CDn_m Matrix cd = astr.cd sxaddpar, newhd, 'CD1_1', cd[0,0]*box sxaddpar, newhd, 'CD1_2', cd[0,1]*box sxaddpar, newhd, 'CD2_1', cd[1,0]*box sxaddpar, newhd, 'CD2_2', cd[1,1]*box endelse endif bscale = sxpar( oldhd, 'BSCALE') if ( bscale NE 0 ) and ( bscale NE 1) then $ sxaddpar, newhd, 'BSCALE', bscale*pix_ratio, ' CALIBRATION FACTOR' bzero = sxpar( oldhd, 'BZERO') if ( bzero NE 0) then sxaddpar, newhd, 'BZERO', bzero*pix_ratio, $ ' ADDITIVE CONST FOR CALIB' if npar LT 4 then oldhd = newhd return end