Conversion of standardized ReadMe file for
file /./ftp/cats/J/PASP/106/745 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-19
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/PASP/106/745 The Spectrum of IC 418 (Hyung+ 1994)
*================================================================================
*The Spectrum of the Planetary Nebula, IC 418
* Hyung S., Aller L. H., and Feibelman W. A.
* <Publ. Astron. Soc. Pac. 106, 745, (1994)>
* =1994PASP..106..745H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Optical Region line Intensities
integer*4 nr__
parameter (nr__=246) ! Number of records
character*69 ar__ ! Full-size record
real*8 lam_obs ! (0.1nm) *?The observed wavelength
real*8 lam_lab ! (0.1nm) ?The laboratory wavelength
character*13 id ! The line identification
character*8 mult ! The multiplet number
real*4 k ! *?Extinction
real*4 I ! *?Relative intensity to I(Hbeta=100)
real*8 F ! ?The un-corrected flux relative to
* F(Hbeta)=100.
real*4 e_F ! ? Formal root-mean-square error
*Note on lam.obs:
* The observed wavelength in A corrected for the radial velocity,
* V_{rad} = 37.375 km/s.
*Note on k:
* The extinction coefficient, k_{\lambda}, as tabulated from
* equations given by Seaton (1979MNRAS.187p..73S)
*Note on I:
* the flux I(lam) relative to I(Hbeta) =100 corrected for
* interstellar extinction, C = log I(H beta)/F(H beta) = 0.21, a
* value derived by comparing reliable Balmer and Paschen lines. that
* is, the extinction at lambda 4861 is 0.21 dex.
C=============================================================================
C Loading file 'table5.dat' ! Optical Region line Intensities
C Format for file interpretation
1 format(
+ F8.2,1X,F8.2,2X,A13,1X,A8,1X,F6.3,1X,F6.2,1X,F7.2,2X,F4.1)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,246
read(1,'(A69)')ar__
read(ar__,1)lam_obs,lam_lab,id,mult,k,I,F,e_F
if(ar__(1:8) .EQ. '') lam_obs = rNULL__
if(ar__(10:17) .EQ. '') lam_lab = rNULL__
if(ar__(43:48) .EQ. '') k = rNULL__
if(ar__(50:55) .EQ. '') I = rNULL__
if(ar__(57:63) .EQ. '') F = rNULL__
if(ar__(66:69) .EQ. '') e_F = rNULL__
c ..............Just test output...........
write(6,1)lam_obs,lam_lab,id,mult,k,I,F,e_F
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end