FORTRAN Generation
(/./ftp/cats/J/AZh/85/794)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AZh/85/794 into FORTRAN code for loading all data files into arrays.

Note that special values are assigned to unknown or unspecified numbers (also called NULL numbers); when necessary, the coordinate components making up the right ascension and declination are converted into floating-point numbers representing these angles in degrees.



      program load_ReadMe
C=============================================================================
C  F77-compliant program generated by readme2f_1.81 (2015-09-23), on 2024-Apr-19
C=============================================================================
*  This code was generated from the ReadMe file documenting a catalogue
*  according to the "Standard for Documentation of Astronomical Catalogues"
*  currently in use by the Astronomical Data Centers (CDS, ADC, A&A)
*  (see full documentation at URL http://vizier.u-strasbg.fr/doc/catstd.htx)
*  Please report problems or questions to   
C=============================================================================

      implicit none
*  Unspecified or NULL values, generally corresponding to blank columns,
*  are assigned one of the following special values:
*     rNULL__    for unknown or NULL floating-point values
*     iNULL__    for unknown or NULL   integer      values
      real*4     rNULL__
      integer*4  iNULL__
      parameter  (rNULL__=--2147483648.)  	! NULL real number
      parameter  (iNULL__=(-2147483647-1))	! NULL int  number
      integer    idig			! testing NULL number

C=============================================================================
Cat. J/AZh/85/794      UBVRH{alpha} photometry on 5 galaxies          (Gusev+, 2008)
*================================================================================
*Age and interstellar absorption in young star-formation regions in the galaxies
*NGC 1068, NGC 4449, NGC 4490, NGC 4631, and NGC 4656/57 derived from multicolor
*photometry.
*    Gusev A.S., Myakutin V.I., Piskunov A.E., Sakhibov F.K., Khramtsova M.S.
*    <Astron. Zh. 85, 794 (2008)>
*    =2008AZh....85..794G
*    =2008ARep...52..714G
C=============================================================================

C  Internal variables

      integer*4 i__

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table1.dat'	! Photometry of star formation complexes (SFCs) 
                             in galaxies

      integer*4 nr__
      parameter (nr__=170)	! Number of records
      character*64 ar__   	! Full-size record

      character*8   Galaxy     (nr__) ! Galaxy name
      character*3   m_Galaxy   (nr__) ! [/57 ] For Galaxy = NGC 4556/57
      integer*4     HII        (nr__) ! Giant HII region number within the cluster
      real*4        U_B        (nr__) ! (mag) ?=- U-B colour index
      real*4        B_V        (nr__) ! (mag) ?=- B-V colour index
      real*4        V_R        (nr__) ! (mag) ?=- V-R colour index
      real*4        LCI        (nr__) ! (mag) ?=- Lyman continuum index (1)
      real*4        Bmag       (nr__) ! (mag) B magnitude
      real*4        D          (nr__) ! (arcsec) Size of the image of the object in the
*                                   H{alpha}+[NII] filter
      real*4        AV         (nr__) ! (mag) ? Interstellar absorption in V band
      real*4        logt       (nr__) ! ([yr]) ? Age estimate
      real*4        Delta      (nr__) ! (mag) ? Error in the colours corrected for the
*                                    interstellar absorption (2)
*Note (1): LCI=2-log(F(Ha+[NII])/F(B)), where F(Ha+[NII] is the flux in
*     close hydrogen and nitrogen emission lines and F(B) the flux in the
*     stellar continuum in the B Band.
*Note (2): Error is deviations of color indices corrected for interstellar
*     absorption from theoretical color indices for the nearest node of
*     evolutionary model grid.

C=============================================================================

C  Loading file 'table1.dat'	! Photometry of star formation complexes (SFCs) 
*                             in galaxies

C  Format for file interpretation

    1 format(
     +  A8,A3,1X,I2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.1,
     +  1X,F4.2,1X,F4.2,1X,F4.2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,170
        read(1,'(A64)')ar__
        read(ar__,1)
     +  Galaxy(i__),m_Galaxy(i__),HII(i__),U_B(i__),B_V(i__),V_R(i__),
     +  LCI(i__),Bmag(i__),D(i__),AV(i__),logt(i__),Delta(i__)
        if (idig(ar__(16:20)).EQ.0) U_B(i__) =  rNULL__
        if (idig(ar__(22:26)).EQ.0) B_V(i__) =  rNULL__
        if (idig(ar__(28:32)).EQ.0) V_R(i__) =  rNULL__
        if (idig(ar__(34:38)).EQ.0) LCI(i__) =  rNULL__
        if(ar__(51:54) .EQ. '') AV(i__) = rNULL__
        if(ar__(56:59) .EQ. '') logt(i__) = rNULL__
        if(ar__(61:64) .EQ. '') Delta(i__) = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  Galaxy(i__),m_Galaxy(i__),HII(i__),U_B(i__),B_V(i__),V_R(i__),
     +  LCI(i__),Bmag(i__),D(i__),AV(i__),logt(i__),Delta(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================
      stop
      end

C Locate position of first digit in string; or return 0
      integer function idig(c)
      character*(*) c
      character*1 c1
      integer lc,i
      lc=len(c)
      idig=0
      do i=1,lc
         if(c(i:i).ne.' ') go to 1
      end do
    1 if(i.gt.lc) return
      c1=c(i:i)
      if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1
      if(i.gt.lc) return
      c1=c(i:i)
      if(c1.ge.'0'.and.c1.le.'9') idig=i
      return
      end