Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/609/A108 into FORTRAN code for loading all data files into arrays.
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-Aug-11
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/609/A108 Stellar parameters of Be stars with X-shooter (Shokry+, 2018)
*================================================================================
*Stellar parameters of Be stars observed with X-shooter.
* Shokry A., Rivinius T., Mehner A., Martayan C., Hummel W., Townsend R.H.D.,
* Merand A., Mota B., Faes D.M., Hamdy M.A., Beheary M.M., Gadallah K.A.K.,
* Abo-Elazm M.S.
* <Astron. Astrophys. 609, A108 (2018)>
* =2018A&A...609A.108S (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table6.dat' ! Parameters of stellar models used to measure the
theoretical values of the Balmer discontinuity
parameters used in the BCD method, D_star and
lambda_1
integer*4 nr__
parameter (nr__=3450) ! Number of records
character*84 ar__ ! Full-size record
character*30 Ident (nr__) ! Approximate spectral type (ident)
real*4 Lstar (nr__) ! ([Lsun]) log of the stellar luminosity (L_star)
real*4 Mstar (nr__) ! (Msun) Stellar mass (M_star)
real*4 Rpole (nr__) ! Polar radius (R_pole)
integer*4 Teff (nr__) ! (K) Stellar effective temperature (T_eff)
real*4 loggpole (nr__) ! ([cm/s2]) log of polar gravity (logg_pole)
real*4 omega (nr__) ! Critical fraction in linear velocity (omega)(1)
integer*4 vsini (nr__) ! (km/s) Stellar projected rotational velocity (vsini)
real*4 Dstar (nr__) ! BCD parameter D_star (D_star)
real*4 lambda1 (nr__) ! (0.1nm) BCD parameter lambda_1 (lambda1)
integer*4 respow (nr__) ! Spectral resolving power for which the BCD
* parameters were measured (respow)
*Note (1): note that the values in the paper are given as fraction of angular
* velocity. See epns. 7 and 8 of 2013A&ARv..21...69R for conversion)
C=============================================================================
C Loading file 'table6.dat' ! Parameters of stellar models used to measure the
* theoretical values of the Balmer discontinuity
* parameters used in the BCD method, D_star and
* lambda_1
C Format for file interpretation
1 format(
+ A30,1X,F5.3,1X,F5.2,1X,F4.2,1X,I5,1X,F5.3,1X,F5.3,1X,I3,1X,
+ F4.3,1X,F4.1,1X,I4)
C Effective file loading
open(unit=1,status='old',file=
+'table6.dat')
write(6,*) '....Loading file: table6.dat'
do i__=1,3450
read(1,'(A84)')ar__
read(ar__,1)
+ Ident(i__),Lstar(i__),Mstar(i__),Rpole(i__),Teff(i__),
+ loggpole(i__),omega(i__),vsini(i__),Dstar(i__),lambda1(i__),
+ respow(i__)
c ..............Just test output...........
write(6,1)
+ Ident(i__),Lstar(i__),Mstar(i__),Rpole(i__),Teff(i__),
+ loggpole(i__),omega(i__),vsini(i__),Dstar(i__),lambda1(i__),
+ respow(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end