FORTRAN Generation
(/./ftp/cats/J/A_A/589/A127)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/589/A127 into FORTRAN code for reading data files line by line.

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 2026-May-18
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+A/589/A127  Dimethyl sulfide laboratory um, mm & FIR spectra  (Jabri+, 2016)
*================================================================================
*Laboratory microwave, millimeter wave and far-infrared spectra of dimethyl
*sulfide
*    Jabri A., Nguyen H.V.L., Mouhib H., Tchana F.K., Manceron L., Stahl W.,
*    Kleiner I.
*    <Astron. Astrophys. 589, A127 (2016)>
*    =2016A&A...589A.127J        (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'appenb.dat'	! *Microwave and millimeter-wave range

      integer*4 nr__
      parameter (nr__=602)	! Number of records
      character*92 ar__   	! Full-size record

      integer*4     v111        ! [0/1] Observed v11 upper state (G1)
      integer*4     v151        ! [0/1] Observed v15 upper state (G1)
      integer*4     J1          ! Observed J upper state
      integer*4     Ka1         ! Observed Ka upper state
      integer*4     Kc1         ! Observed Kc upper state
      integer*4     v110        ! [0/1] Observed v11 lower state (G1)
      integer*4     v150        ! [0/1] Observed v15 lower state (G1)
      integer*4     J0          ! Observed J lower state
      integer*4     Ka0         ! Observed Ka lower state
      integer*4     Kc0         ! Observed Kc lower state
      real*8        Freq_Obs    ! (MHz) Observed line frequency
      integer*4     e_Freq_Obs  ! (kHz) rms uncertainty on Freq.Obs (G2)
      real*8        Freq_Cal    ! (MHz) Calculated line frequency
      real*4        e_Freq_Cal  ! (MHz) ? rms uncertainty on Freq.Cal
      real*4        O_C         ! (MHz) Difference between the experimental and
*                                   calculated frequencies
      real*8        S_mu__2     ! (D+2) Calculated line strength (3)
      real*8        E0          ! (cm-1) Upper state energy including the
*                                   zero-point torsional energy
      real*8        E1          ! (cm-1) Lower state energy including the
*                                   zero-point torsional energy
      character*2   Sym         ! Symmetry species in the
*                                   C^-^_3v_ X c^+^_3v_ direct product (4)
*Note (3): Note that the line strengths are given as S*mu**2. To obtain
*  intensities the line strengths need to be multiplied by appropriate
*  statistical weights, Boltzmann factor and divided by the total partition
*  function (see appendix C).
*Note (4): The spin-weight statistics for the transitions AA: EE: AE: EA depend
*  on the parity of KaKc, i.e. 6:16:4:2 for KaKc: ee-oo and
*  10:16:4:6 for KaKc: eo-oe (Vacherand et al. 1987).

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

C  Declarations for 'appenc.dat'	! *Far-infrared range

      integer*4 nr__1
      parameter (nr__1=578)	! Number of records
      character*72 ar__1  	! Full-size record

      integer*4     v111_1      ! [0] Observed v11 upper state
      integer*4     v151_1      ! [1] Observed v15 upper state
      integer*4     J1_1        ! J upper state
      integer*4     Ka1_1       ! Ka upper state
      integer*4     Kc1_1       ! Kc upper state
      integer*4     v110_1      ! [0] v11 lower state
      integer*4     v150_1      ! [0] v15 lower state
      integer*4     J0_1        ! J lower state
      integer*4     Ka0_1       ! Ka lower state
      integer*4     Kc0_1       ! Kc lower state
      real*8        Freq_Obs_1  ! (MHz) Observed line frequency
      integer*4     e_Freq_Obs_1 ! (kHz) rms uncertainty on Freq.Obs
      real*8        Freq_Cal_1  ! (MHz) Calculated line frequency
      real*8        O_C_1       ! (MHz) Difference between the experimental and
*                                   calculated frequencies
      real*8        E0_1        ! (cm-1) Upper state energy including the zero-point
*                                   torsional energy calculated at 187.6294cm^-1^
      real*8        E1_1        ! (cm-1) Lower state energy including the zero-point
*                                   torsional energy calculated at 187.6294cm^-1^
      character*2   Sym_1       ! Symmetry species in the
*                                   C^-^_3v_ X c^+^_3v_ direct product

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

C  Declarations for 'appene.dat'	! A line-list of all rotational transitions
                                  reliably predicted between 0 and 300GHz with
                                  the set of spectroscopic parameters
                                  determined in Appendix A

      integer*4 nr__2
      parameter (nr__2=7158)	! Number of records
      character*94 ar__2  	! Full-size record

      integer*4     v111_2      ! [0] Observed v11 upper state (G1)
      integer*4     v151_2      ! [0] Observed v15 upper state (G1)
      integer*4     J1_2        ! Observed J upper state
      integer*4     Ka1_2       ! Observed Ka upper state
      integer*4     Kc1_2       ! Observed Kc upper state
      integer*4     v110_2      ! [0] Observed v11 lower state (G1)
      integer*4     v150_2      ! [0] Observed v15 lower state (G1)
      integer*4     J0_2        ! Observed J lower state
      integer*4     Ka0_2       ! Observed Ka lower state
      integer*4     Kc0_2       ! Observed Kc lower state
      real*8        Freq_Obs_2  ! (MHz) ? Observed line frequency
      integer*4     e_Freq_Obs_2 ! (kHz) ? rms uncertainty on Freq.Obs (G2)
      real*8        Freq_Cal_2  ! (MHz) Calculated line frequency
      real*4        e_Freq_Cal_1 ! (MHz) rms uncertainty on Freq.Cal
      real*4        O_C_2       ! (MHz) ? Difference between the experimental and
*                                     calculated frequencies
      real*8        Smu_2       ! (D+2) Calculated line strength
      real*8        E0_2        ! (cm-1) Upper state energy including the
*                                   zero-point torsional energy
      real*8        E1_2        ! (cm-1) Lower state energy including the
*                                   zero-point torsional energy
      character*2   Sym_2       ! Symmetry species in the
*                                   C^-^_3v_ X c^+^_3v_ direct product

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

C  Loading file 'appenb.dat'	! *Microwave and millimeter-wave range

C  Format for file interpretation

    1 format(
     +  I1,I1,1X,I2,1X,I2,1X,I2,1X,I1,I1,1X,I2,1X,I2,1X,I2,1X,F10.3,
     +  1X,I3,1X,F10.3,1X,F5.3,1X,F6.3,1X,F8.5,1X,F8.4,1X,F8.4,1X,A2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'appenb.dat')
      write(6,*) '....Loading file: appenb.dat'
      do i__=1,602
        read(1,'(A92)')ar__
        read(ar__,1)
     +  v111,v151,J1,Ka1,Kc1,v110,v150,J0,Ka0,Kc0,Freq_Obs,e_Freq_Obs,
     +  Freq_Cal,e_Freq_Cal,O_C,S_mu__2,E0,E1,Sym
        if(ar__(51:55) .EQ. '') e_Freq_Cal = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  v111,v151,J1,Ka1,Kc1,v110,v150,J0,Ka0,Kc0,Freq_Obs,e_Freq_Obs,
     +  Freq_Cal,e_Freq_Cal,O_C,S_mu__2,E0,E1,Sym
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'appenc.dat'	! *Far-infrared range

C  Format for file interpretation

    2 format(
     +  I1,I1,1X,I2,1X,I2,1X,I2,1X,I1,I1,1X,I2,1X,I2,1X,I2,1X,F8.4,1X,
     +  I1,1X,F8.4,1X,F7.4,1X,F8.4,1X,F8.4,1X,A2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'appenc.dat')
      write(6,*) '....Loading file: appenc.dat'
      do i__=1,578
        read(1,'(A72)')ar__1
        read(ar__1,2)
     +  v111_1,v151_1,J1_1,Ka1_1,Kc1_1,v110_1,v150_1,J0_1,Ka0_1,Kc0_1,
     +  Freq_Obs_1,e_Freq_Obs_1,Freq_Cal_1,O_C_1,E0_1,E1_1,Sym_1
c    ..............Just test output...........
        write(6,2)
     +  v111_1,v151_1,J1_1,Ka1_1,Kc1_1,v110_1,v150_1,J0_1,Ka0_1,Kc0_1,
     +  Freq_Obs_1,e_Freq_Obs_1,Freq_Cal_1,O_C_1,E0_1,E1_1,Sym_1
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'appene.dat'	! A line-list of all rotational transitions
*                                  reliably predicted between 0 and 300GHz with
*                                  the set of spectroscopic parameters
*                                  determined in Appendix A

C  Format for file interpretation

    3 format(
     +  I1,I1,1X,I2,1X,I3,1X,I2,1X,I1,I1,1X,I2,1X,I3,1X,I2,1X,F10.3,
     +  1X,I3,1X,F10.3,1X,F5.3,1X,F6.3,1X,F8.5,1X,F8.4,1X,F8.4,1X,A2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'appene.dat')
      write(6,*) '....Loading file: appene.dat'
      do i__=1,7158
        read(1,'(A94)')ar__2
        read(ar__2,3)
     +  v111_2,v151_2,J1_2,Ka1_2,Kc1_2,v110_2,v150_2,J0_2,Ka0_2,Kc0_2,
     +  Freq_Obs_2,e_Freq_Obs_2,Freq_Cal_2,e_Freq_Cal_1,O_C_2,Smu_2,
     +  E0_2,E1_2,Sym_2
        if(ar__2(27:36) .EQ. '') Freq_Obs_2 = rNULL__
        if(ar__2(38:40) .EQ. '') e_Freq_Obs_2 = iNULL__
        if(ar__2(59:64) .EQ. '') O_C_2 = rNULL__
c    ..............Just test output...........
        write(6,3)
     +  v111_2,v151_2,J1_2,Ka1_2,Kc1_2,v110_2,v150_2,J0_2,Ka0_2,Kc0_2,
     +  Freq_Obs_2,e_Freq_Obs_2,Freq_Cal_2,e_Freq_Cal_1,O_C_2,Smu_2,
     +  E0_2,E1_2,Sym_2
c    .......End.of.Just test output...........
      end do
      close(1)

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