FORTRAN Generation
(/./ftp/cats/J/A_A/597/A22)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/597/A22 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/597/A22       Massive O- and B-type stars velocities   (Simon-Diaz+, 2017)
*================================================================================
*The IACOB project.
*III. New observational clues to understand macroturbulent broadening in
*massive O- and B-type stars.
*    Simon-Diaz S., Godart M., Castro N., Herrero A., Aerts C., Puls J.,
*    Telting J., Grassitelli L.
*    <Astron. Astrophys. 597, A22 (2017)>
*    =2017A&A...597A..22S        (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'tablea1.dat'	! List of stars considered for this paper

      integer*4 nr__
      parameter (nr__=431)	! Number of records
      character*80 ar__   	! Full-size record

      character*13  Target      ! HD number of the star
      character*17  SpType      ! Spectral type (1)
      character*5   Line        ! Line used to determine the line-broadening
*                                  parameters
      integer*4     S_Nc        ! Signal-to-noise ratio of the adjacent continuum
      integer*4     EW          ! (0.1pm) Equivalent width of the line
      integer*4     vsiniF      ! (km/s) Projected rotational velocity as derived from 
*                                  the Fourier transform (FT) approach
      integer*4     vsiniG      ! (km/s) Projected rotational velocity as derived from 
*                                  the goodness of fit (GOF) approach
      character*1   l_vmac      ! Limit flag on vmac
      integer*4     vmac        ! (km/s) Macroturbulent velocity as derived from the 
*                                  goodness of fit (GOF) approach
      real*4        RSk         ! Relative skewness of the line profile as 
*                                  derived using Eq. 1 in the paper (2)
      real*4        e_RSk       ! rms uncertainty on RSk
      real*4        logTeff     ! ([K]) ?=- Effective temperature
      real*4        logL        ! ([Lsun]) ?=- Luminosity (L=Teff^4^/g)
*Note (1): Spectral classifications must be handled with caution since they come
*  from various sources, not all of which are equally reliable.
*Note (2): Relative skewness, RSk=<v^3^>/(<v^2^>^3/2^), where v^2^ and v^3^ are
*  the second and third normalized central moments of a spectral line,
*  see Equation (1), Sect. 3.2 of the paper.

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

C  Loading file 'tablea1.dat'	! List of stars considered for this paper

C  Format for file interpretation

    1 format(
     +  A13,1X,A17,1X,A5,2X,I3,1X,I3,1X,I3,1X,I3,1X,A1,I3,1X,F5.2,1X,
     +  F4.2,1X,F4.2,1X,F4.2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'tablea1.dat')
      write(6,*) '....Loading file: tablea1.dat'
      do i__=1,431
        read(1,'(A80)')ar__
        read(ar__,1)
     +  Target,SpType,Line,S_Nc,EW,vsiniF,vsiniG,l_vmac,vmac,RSk,
     +  e_RSk,logTeff,logL
        if (idig(ar__(72:75)).EQ.0) logTeff =  rNULL__
        if (idig(ar__(77:80)).EQ.0) logL =  rNULL__
c    ..............Just test output...........
        write(6,1)
     +  Target,SpType,Line,S_Nc,EW,vsiniF,vsiniG,l_vmac,vmac,RSk,
     +  e_RSk,logTeff,logL
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