C @(#)irsflat.for 17.1.1.1 (ES0-DMD) 01/25/02 17:53:06 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 Massachusetss Ave, Cambridge, C MA 02139, USA. C C Corresponding 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 C+++++++++++++++++++++++++++++++++++++++++++++++++++++++ C C.COPYRIGHT (C) 1992 European Southern Observatory C.IDENT .for C.AUTHOR E. Oliva, Firenze-Arcetri C.KEYWORDS Spectroscopy, IRSPEC C C.PURPOSE Execute command ... C C.ALGORITHM C C C.INPUT/OUTPUT C C C.VERSION 1.0 Creation 02.09.1992 E. Oliva C C------------------------------------------------------- C PROGRAM IRFLAT IMPLICIT REAL(A-H,O-Z) IMPLICIT INTEGER(I-N) CHARACTER*64 CUNIT CHARACTER*72 IDENT INTEGER*8 INPNTR,OUPNTR INTEGER NPIX(2),MMPIX(2) REAL CUTS(2) DOUBLE PRECISION START(2),STEP(2) COMMON /VMR/ MADRID(1) INCLUDE 'MID_INCLUDE:ST_DEF.INC' INCLUDE 'MID_INCLUDE:ST_DAT.INC' DATA MAXDIM/2/ IRET=1 CALL STSPRO('IRFLAT') C C GET INPUT FRAME AND MAP IT C CHECK ALSO WHETHER IT IS A 2D FRAME..... C CALL STIGET('middummb',D_R4_FORMAT,F_I_MODE,F_IMA_TYPE,MAXDIM, , NAXIS,NPIX,START,STEP, , IDENT,CUNIT,INPNTR,NIN,ISTAT) IF(NAXIS.NE.2) + CALL STETER(1,'Input frame must be 2-D') C C GET OUTPUT FRAME AND MAP IT C CALL STIPUT('middummc',D_R4_FORMAT,F_O_MODE,F_IMA_TYPE, , NAXIS,NPIX,START,STEP, , IDENT,CUNIT,OUPNTR,NOU,ISTAT) C C GET key TO DEFINE threshold value C CALL STKRDR('thres',1,1,IRET,THRES,KUNIT,KNUL,ISTAT) C C GET key TO DEFINE the value to which vignetted pixels must be C forced. C CALL STKRDR('vignet',1,1,IRET,VIGNET,KUNIT,KNUL,ISTAT) C C CALL ROUTINE WHICH which divides by a constant and modifies vignetted C rows C CALL NORMAL(MADRID(INPNTR),MADRID(OUPNTR), , NPIX(1),NPIX(2),THRES,VIGNET) C C Define and write cuts of output file C CALL MNMX(MADRID(OUPNTR),NPIX,CUTS,MMPIX) CALL STDWRR(NOU,'LHCUTS',CUTS,3,2,KUNIT,ISTAT) C C RELEASE FILES, UPDATE KEYWORDS AND EXIT C CALL STSEPI END C C C SUBROUTINE NORMAL(A,B,NX,NY,THRES,VIGNET) C C divides the input frame by the average C value of the central 10 rows (=AVER_CENT) C In the computation of AVER_CENT the first and last 2 pixels C of each row are not considered to avoid edge effects. C C All rows with average signal