FORTRAN Generation
(/./ftp/cats/J/A_A/694/A26)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/694/A26 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-Sep-10
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/694/A26       Radio flux variability in UCHII regions        (Yang+, 2025)
*================================================================================
*Dynamic massive star formation: Radio flux variability in UCHII regions.
*    Yang A.Y., Thompson M.A., Urquhart J.S., Brunthaler A., Menten K.M.,
*    Gong Y., Tsai C.-W., Patel A.L., Li D., Cotton W.D.
*    <Astron. Astrophys. 694, A26 (2025)>
*    =2025A&A...694A..26Y        (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! The sample of 38 UCHII with radio flux variations

      integer*4 nr__
      parameter (nr__=38)	! Number of records
      character*117 ar__   	! Full-size record

C  J2000 position composed of: RAdeg DEdeg
      character*17  Name        ! Galactic name (GLLL.llll+BB.bbbb)
      real*8        GLON        ! (deg) Galactic longitude
      real*8        GLAT        ! (deg) Galactic latitude
      real*8        RAdeg       ! (deg) Right Ascension (J2000)
      real*8        DEdeg       ! (deg) Declination (J2000)
      real*4        SpeakG      ! (mJy/beam) Peak flux density GLOSTAR at 5GHz
      real*4        e_SpeakG    ! (mJy/beam) Uncertainty in SpeakG at 5GHz
      real*4        SpeakC      ! (mJy/beam) Peak flux density CORNISH at 5GHz
      real*4        e_SpeakC    ! (mJy/beam) Uncertainty in SpeakC at 5GHz
      real*4        thetaS      ! (arcsec) Angular scale (geometric average)
      real*4        thetadcon   ! (arcsec) Deconvolved angular scale
      character*1   n_thetadcon ! [*] Note on thetadcon (1)
      real*4        Diam        ! (pc) []?=- Linear diameter of the source
      real*4        Dist        ! (pc) []?=- Heliocentric distance
      real*4        fvar        ! (pc) ?=- Flux variation fraction
      real*4        alpha       ! ?=- Spectral index fitted from the
*                                      sub-images of GLOSTAR (2)
      real*4        e_alpha     ! ?=- Uncertainty of the spectral index from
*                                      the fitting process of the sub-images of
*                                      GLOSTAR
*Note (1): * refers to unresolved sources that have angular sizes <1.5" and
* their theta_dcon_ are considered the upper-limit values. The upper-limit of
* theta_dcon_ is set to be 0.32", which corresponds to one standard deviation of
* the distribution of beam sizes from the CORNISH survey.
*Note (2): "---" means that the alpha is unreliable and not adopted.

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

C  Loading file 'table1.dat'	! The sample of 38 UCHII with radio flux variations

C  Format for file interpretation

    1 format(
     +  A17,1X,F8.5,1X,F8.5,1X,F9.5,1X,F9.5,1X,F5.2,1X,F4.2,1X,F5.2,
     +  1X,F4.2,1X,F4.2,1X,F4.2,A1,1X,F6.3,1X,F4.1,1X,F5.1,1X,F5.2,1X,
     +  F4.2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,38
        read(1,'(A117)')ar__
        read(ar__,1)
     +  Name,GLON,GLAT,RAdeg,DEdeg,SpeakG,e_SpeakG,SpeakC,e_SpeakC,
     +  thetaS,thetadcon,n_thetadcon,Diam,Dist,fvar,alpha,e_alpha
        if (idig(ar__(90:95)).EQ.0) Diam =  rNULL__
        if (idig(ar__(97:100)).EQ.0) Dist =  rNULL__
        if (idig(ar__(102:106)).EQ.0) fvar =  rNULL__
        if (idig(ar__(108:112)).EQ.0) alpha =  rNULL__
        if (idig(ar__(114:117)).EQ.0) e_alpha =  rNULL__
c    ..............Just test output...........
        write(6,1)
     +  Name,GLON,GLAT,RAdeg,DEdeg,SpeakG,e_SpeakG,SpeakC,e_SpeakC,
     +  thetaS,thetadcon,n_thetadcon,Diam,Dist,fvar,alpha,e_alpha
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