FORTRAN Generation
(/./ftp/cats/J/A_AS/142/467)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_AS/142/467 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/A+AS/142/467     Broadening of metallic lines by H collisions  (Barklem+ 2000)
*================================================================================
*A list of data for the broadening of metallic lines by
*neutral hydrogen collisions.
*     Barklem P.S., Piskunov N., O'Mara B.J.
*    <Astron. Astrophys. Suppl. Ser. 142, 467 (2000)>
*    =2000A&AS..142..467B
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! List of broadening data and other data used in
                                 computation

      integer*4 nr__
      parameter (nr__=4891)	! Number of records
      character*116 ar__   	! Full-size record

      real*4        spec       (nr__) ! Packed element and ionisation stage (1)
      real*8        lambda     (nr__) ! (0.1nm) Air wavelength (Angstroms)
      real*4        lowJ       (nr__) ! Lower level J quantum number
      real*4        uppJ       (nr__) ! Upper level J quantum number
      real*8        lowE       (nr__) ! (eV) Lower level energy in eV (2)
      real*8        uppE       (nr__) ! (eV) Upper level energy in eV (2)
      real*8        lowEcm     (nr__) ! (cm-1) Lower level energy in waves/cm (2)
      real*8        lowlim     (nr__) ! (cm-1) Lower level series limit in waves/cm (2)
      real*8        uppEcm     (nr__) ! (cm-1) Upper level energy in waves/cm (2)
      real*8        upplim     (nr__) ! (cm-1) Upper level series limit in waves/cm (2)
      integer*4     lowl       (nr__) ! Lower level l quantum number
      integer*4     uppl       (nr__) ! Upper level l quantum number
      real*4        sigma      (nr__) ! (2.80x10-21m2) Broadening cross-section in a.u. (3)
      real*4        alpha      (nr__) ! Velocity parameter alpha
      real*4        logGam     (nr__) ! ([rad.cm3/s]) Log of the FWHM per perturber at 10000K
      real*4        Texp       (nr__) ! Temperature dependence exponent 
*                                           (1-alpha)/2
*Note (1): The element and ionisation stage are packed into one parameter
*          given by Z + (Z-N)*0.01 where Z is the atomic number of the
*          element, and N is the total number of electrons.
*Note (2): A value of -1.0 indicates that the data was computed directly
*          and not interpolated from the grids.  This occurs for all lines
*          of singly ionised species and a few important neutral species
*          lines where the states lie just off the grid.
*Note (3): The atomic unit of cross-section is a_0_^2^, Bohr radius squared
*           (the Bohr radius is the constant 
*                a_0_ = {epsilon}_0_ h^2^/({pi} m e^2^)
*            from Permittivity, Planck, electron mass and charge constants)

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

C  Loading file 'table1.dat'	! List of broadening data and other data used in
*                                 computation

C  Format for file interpretation

    1 format(
     +  F5.2,1X,F10.3,1X,F4.1,1X,F4.1,1X,F7.3,1X,F7.3,1X,F10.3,1X,
     +  F10.3,1X,F10.3,1X,F10.3,1X,I1,1X,I1,1X,F6.0,1X,F5.3,1X,F6.3,
     +  1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,4891
        read(1,'(A116)')ar__
        read(ar__,1)
     +  spec(i__),lambda(i__),lowJ(i__),uppJ(i__),lowE(i__),uppE(i__),
     +  lowEcm(i__),lowlim(i__),uppEcm(i__),upplim(i__),lowl(i__),
     +  uppl(i__),sigma(i__),alpha(i__),logGam(i__),Texp(i__)
c    ..............Just test output...........
        write(6,1)
     +  spec(i__),lambda(i__),lowJ(i__),uppJ(i__),lowE(i__),uppE(i__),
     +  lowEcm(i__),lowlim(i__),uppEcm(i__),upplim(i__),lowl(i__),
     +  uppl(i__),sigma(i__),alpha(i__),logGam(i__),Texp(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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