FORTRAN Generation
(/./ftp/cats/J/AJ/132/1851)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AJ/132/1851 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-Apr-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/AJ/132/1851       Arecibo obs. of formaldehyde in L1551    (Araya+, 2006)
*================================================================================
*Arecibo observations of formaldehyde in L1551.
*    Araya E., Hofner P., Olmi L., Kurtz S., Linz H.
*   <Astron. J., 132, 1851-1858 (2006)>
*   =2006AJ....132.1851A
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Model Results

      integer*4 nr__
      parameter (nr__=64)	! Number of records
      character*60 ar__   	! Full-size record

      integer*4     oRA         ! (arcmin) Offset along Right Ascension (1)
      integer*4     oDE         ! (arcmin) Offset along Declination (1)
      real*4        Tex0        ! (K) Excitation temperature lower limit
      real*4        Tex1        ! (K) Excitation temperature upper limit
      real*4        tau0        ! Optical depth lower limit
      real*4        tau1        ! Optical depth upper limit
      real*4        DelV0       ! (km/s) Line width lower limit
      real*4        DelV1       ! (km/s) Line width upper limit
      real*4        VLSR0       ! (km/s) The F=2-2 hyperfine component
*                                     LSR velocity, lower limit
      real*4        VLSR1       ! (km/s) The F=2-2 hyperfine component
*                                     LSR velocity, upper limit
      real*4        chi2        ! {chi}^2^ value (2)
      real*4        Dchi2       ! ? Different {chi}^2^ value for
*                                    DelV and VLSR ranges (3)
      character*1   Wing        ! [c] Presence of wings (4)
*Note (1): Reference position is 04:31:21.8+18:05:54 (J2000).
*Note (2): When {chi}^2^ values of less than 23.5 were obtained, we explored
*     the convergence of the parameters at fixed {chi}^2^ levels, i.e.,
*     {chi}^2^=4.72, 7.78, 9.70, 13.3, 16.3, and 23.5 levels, which
*     correspond to confidence levels of 68.3%, 90.0%, 95.4%, 99.0%, 99.73%,
*     and 99.99% for a four-degrees-of-freedom {chi}^2^ fitting (Press et
*     al., 1999, Numerical Recipes in C (2nd ed.; Cambridge: Cambridge Univ.
*     Press) ). When convergence better than the {chi}^2^=23.5 value was not
*     achieved, then arbitrary {chi}^2^ levels were used.
*Note (3): In some cases the DelV and VLSR parameters converge within given
*     {chi}^2^ value, whereas the tau and Tex parameters show multiple
*     solutions for the same {chi}^2^ contour level. For those cases we
*     report DelV and VLSR ranges for a different {chi}^2^ contour level
*     than the one used to obtain the tau and Tex ranges.
*Note (4): Presence of wings precluded a reliable fit of the complete line
*     profile. See lower panels of Figure 6 as example.

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

C  Loading file 'table1.dat'	! Model Results

C  Format for file interpretation

    1 format(
     +  I2,1X,I2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,
     +  F4.2,1X,F4.2,1X,F6.2,1X,F5.2,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,64
        read(1,'(A60)')ar__
        read(ar__,1)
     +  oRA,oDE,Tex0,Tex1,tau0,tau1,DelV0,DelV1,VLSR0,VLSR1,chi2,
     +  Dchi2,Wing
        if(ar__(54:58) .EQ. '') Dchi2 = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  oRA,oDE,Tex0,Tex1,tau0,tau1,DelV0,DelV1,VLSR0,VLSR1,chi2,
     +  Dchi2,Wing
c    .......End.of.Just test output...........
      end do
      close(1)

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