Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/518/A29 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-Jun-08
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/518/A29 Distribution of WR stars in 2 nearby galaxies (Leloudas+, 2010)
*================================================================================
*Do Wolf-Rayet stars have similar locations in hosts as type Ib/c supernovae and
*long gamma-ray bursts?
* Leloudas G., Sollerman J., Levan A.J., Fynbo J.P.U., Malesani D.,
* Maund J.R.
* <Astron. Astrophys., 518, A29-29 (2010)>
* =2010A&A...518A..29L
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! Fractional fluxes at the locations of the WR stars
integer*4 nr__
parameter (nr__=309) ! Number of records
character*28 ar__ ! Full-size record
character*8 Gal ! Galaxy name (M 83 or NGC 1313)
integer*4 Region ! Region sequential number within the galaxy (1)
character*5 SpT ! WR subtype or "cand." for candidate region (2)
character*1 n_SpT ! [a] a for stars classified as WN5-6 and
* included in the WNE distribution
integer*4 Nstar ! ? Number of stars in the region with this
* WR sub-type
real*4 FF ! Fractional flux (relative surface brightness) (3)
*Note (1): We follow the exact numbering of Hadfield et al. (2005, Cat.
* J/A+A/439/265, <[HCS2005] NNN> in Simbad) and Hadfield & Crowther
* (2007, Cat. J/MNRAS/381/418, <[HC2007] NN> in Simbad). Additional
* info (e.g. fluxes, errors in star numbers) can be found in these
* references.
*Note (2): Subtypes as follows:
* WCE = early WC type
* WCL = late WC type
* WNE = early WN type
* WNL = late WN type
* cand. = candidate region
*Note (3): These fractional fluxes refer to a binning of 15 and 19 for the
* images of M 83 and NGC 1313 we have used, respectively. Although we
* have shown that the results do not change significantly with the
* choice of binning, individual fractional fluxes can vary.
C=============================================================================
C Loading file 'tablea1.dat' ! Fractional fluxes at the locations of the WR stars
C Format for file interpretation
1 format(A8,1X,I3,1X,A5,1X,A1,I3,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea1.dat')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,309
read(1,'(A28)')ar__
read(ar__,1)Gal,Region,SpT,n_SpT,Nstar,FF
if(ar__(21:23) .EQ. '') Nstar = iNULL__
c ..............Just test output...........
write(6,1)Gal,Region,SpT,n_SpT,Nstar,FF
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end