FORTRAN Generation
(/./ftp/cats/J/A_A/595/A88)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/595/A88 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 2024-Mar-29
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/595/A88       G345.45+1.50 ^13^CO(3-2) clumps      (Lopez-Calderon+, 2016)
*================================================================================
*G345.45+1.50: an expanding ring-like structure with massive star formation.
*    Lopez-Calderon C., Bronfman L., Nyman L.-A., Garay G.,
*    de Gregorio-Monsalvo I., Bergman P.
*   <Astron. Astrophys., 595, A88 (2016)>
*   =2016A&A...595A..88L    (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'tablef1.dat'	! Physical properties of the ^13^CO clumps

      integer*4 nr__
      parameter (nr__=104)	! Number of records
      character*62 ar__   	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg       ! (deg) Right Ascension J2000
      real*8        DEdeg       ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      integer*4     Seq         ! [1/104] Sequential number
      integer*4     RAh         ! (h) Right ascension (J2000)
      integer*4     RAm         ! (min) Right ascension (J2000)
      real*4        RAs         ! (s) Right ascension (J2000)
      character*1   DE_         ! Declination sign (J2000)
      integer*4     DEd         ! (deg) Declination (J2000)
      integer*4     DEm         ! (arcmin) Declination (J2000)
      real*4        DEs         ! (arcsec) Declination (J2000)
      real*4        Dc          ! (pc) Clump diameter
      real*4        Mc          ! (Msun) Clump mass
      real*4        DVc         ! (km/s) Clump ^13^CO line velocity width
      real*4        nc          ! (cm-3) Clump ^13^CO density
      real*4        Nc_1        ! (cm-2) Clump ^13^CO column density
      character*1   Type        ! [ABC] Clump type (1)
      character*1   B_E         ! [Y/N] indicates if clumps are candidates to be
*                                   experimenting collapse ({xi}max>=6.5)
*Note (1): The clumps are classified into three types as follows:
*   A = clumps have a counterpart seen in infrared and millimeter wavelengths
*   B = clumps only have a counterpart in the 1.2mm continuum
*   C = clumps are only seen in ^13^CO.

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

C  Loading file 'tablef1.dat'	! Physical properties of the ^13^CO clumps

C  Format for file interpretation

    1 format(
     +  I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F3.1,1X,E6.2,
     +  1X,F3.1,1X,E6.2,1X,E7.2,1X,A1,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablef1.dat')
      write(6,*) '....Loading file: tablef1.dat'
      do i__=1,104
        read(1,'(A62)')ar__
        read(ar__,1)
     +  Seq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Dc,Mc,DVc,nc,Nc_1,Type,B_E
        RAdeg = rNULL__
        DEdeg = rNULL__
c  Derive coordinates RAdeg and DEdeg from input data
c  (RAdeg and DEdeg are set to rNULL__ when unknown)
        if(RAh .GT. -180) RAdeg=RAh*15.
        if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
        if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
        if(DEd .GE. 0) DEdeg=DEd
        if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
        if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
        if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c    ..............Just test output...........
        write(6,1)
     +  Seq,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Dc,Mc,DVc,nc,Nc_1,Type,B_E
        write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c    .......End.of.Just test output...........
      end do
      close(1)

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