Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/694/A248 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-May-17
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/A248 Metallicity spread and dispersion among P1 stars (Latour+, 2025)
*================================================================================
*A stellar census in globular clusters with MUSE.
*Metallicity spread and dispersion among first-population stars.
* Latour M., Kamann S., Martocchia S., Husser T.-O., Saracino S., Dreizler S.
* <Astron. Astrophys. 694, A248 (2025)>
* =2025A&A...694A.248L (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Properties of the RGB stars in our spectral sample
integer*4 nr__
parameter (nr__=8382) ! Number of records
character*132 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 Source (nr__) ! Star identification number
real*8 RAdeg (nr__) ! (deg) Right ascension (J2000)
real*8 DEdeg (nr__) ! (deg) Declination (J2000)
character*7 Cluster (nr__) ! Cluster name
real*4 v_M_H_ (nr__) ! ([Sun]) Metallicity
real*4 e__M_H_ (nr__) ! ([Sun]) Error on the metallicity
integer*4 Teff (nr__) ! (K) Effective temperature
integer*4 e_Teff (nr__) ! (K) Error on the effective temperature
integer*4 SNR (nr__) ! Average signal-to-noise of the Nspec spectra
integer*4 Nspec (nr__) ! Number of spectra used to average
* Teff and [M/H]
real*4 logg (nr__) ! ([cm/s2]) Surface gravity
real*4 e_logg (nr__) ! ([cm/s2]) Error on the surface gravity (1)
real*8 CMx (nr__) ! Delta(F275W,F814W), X-axis position on the
* Chromosome map
real*8 CMy (nr__) ! DeltaC(F275W,F336W,F438W), Y-axis position
* on the Chromosome map
integer*4 P1 (nr__) ! [0/1] =1 if the star belongs to P1
integer*4 P2 (nr__) ! [0/1] =1 if the star belongs to P2
*Note (1): For three clusters there is not uncertainty (=0) on the surface
* gravity measurements because it was obtained with only one set of photometry.
C=============================================================================
C Loading file 'table1.dat' ! Properties of the RGB stars in our spectral sample
C Format for file interpretation
1 format(
+ 1X,I6,2X,F11.7,2X,F11.7,2X,A7,3X,F6.3,2X,F5.3,6X,I4,6X,I2,2X,
+ I3,4X,I2,5X,F5.3,4X,F5.3,2X,F7.4,2X,F7.4,3X,I1,3X,I1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,8382
read(1,'(A132)')ar__
read(ar__,1)
+ Source(i__),RAdeg(i__),DEdeg(i__),Cluster(i__),v_M_H_(i__),
+ e__M_H_(i__),Teff(i__),e_Teff(i__),SNR(i__),Nspec(i__),
+ logg(i__),e_logg(i__),CMx(i__),CMy(i__),P1(i__),P2(i__)
c ..............Just test output...........
write(6,1)
+ Source(i__),RAdeg(i__),DEdeg(i__),Cluster(i__),v_M_H_(i__),
+ e__M_H_(i__),Teff(i__),e_Teff(i__),SNR(i__),Nspec(i__),
+ logg(i__),e_logg(i__),CMx(i__),CMy(i__),P1(i__),P2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end