Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/519/L3 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-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/519/L3 Lithium content of {omega} Cen (Monaco+, 2010)
*================================================================================
*The lithium content of {omega} Centauri. New clues to the cosmological Li
*problem from old stars in external galaxies.
* Monaco L., Bonifacio P., Sbordone L., Villanova S., Pancino E.
* <Astron. Astrophys., 519, L3-3 (2010)>
* =2010A&A...519L...3M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Basic data for MS/SGB stars studied in this paper
integer*4 nr__
parameter (nr__=91) ! Number of records
character*65 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 v_MBS2010_ (nr__) ! Sequential number
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
integer*4 RAm (nr__) ! (min) Right ascension (J2000)
real*4 RAs (nr__) ! (s) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign (J2000)
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Declination (J2000)
real*4 EW (nr__) ! (0.1nm) ?=- Lithium equivalent width
real*4 e_EW (nr__) ! (0.1nm) ?=- rms uncertainty on EW
character*1 l_A_Li (nr__) ! Limit flag on A(Li)
real*4 A_Li (nr__) ! ([Sun]) Lithium abundance (uncertainty=0.1dex)
integer*4 S_N (nr__) ! Signal-to-noise ratio
integer*4 Teff (nr__) ! (K) H{alpha}-based effective temperature
real*4 v_Fe_H_ (nr__) ! ([Sun]) ?=- Estimated metallicity (1)
character*1 n__Fe_H_ (nr__) ! [a] anomalous population SGB-a
* (table2 only, assumed metallicity)
real*4 e__Fe_H_ (nr__) ! ([Sun]) ?=- rms uncertainty on [Fe/H]
*Note (1): For three stars, no [Fe/H] was estimated. These stars were not
* plotted in the bottom panel of Fig. 3.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Basic data for SGB-a stars studied in this paper
integer*4 nr__1
parameter (nr__1=10) ! Number of records
character*65 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 (nr__1) ! (deg) Right Ascension J2000
real*8 DEdeg_1 (nr__1) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 v_MBS2010__1(nr__1) ! Sequential number
integer*4 RAh_1 (nr__1) ! (h) Right ascension (J2000)
integer*4 RAm_1 (nr__1) ! (min) Right ascension (J2000)
real*4 RAs_1 (nr__1) ! (s) Right ascension (J2000)
character*1 DE__1 (nr__1) ! Declination sign (J2000)
integer*4 DEd_1 (nr__1) ! (deg) Declination (J2000)
integer*4 DEm_1 (nr__1) ! (arcmin) Declination (J2000)
real*4 DEs_1 (nr__1) ! (arcsec) Declination (J2000)
real*4 EW_1 (nr__1) ! (0.1nm) ?=- Lithium equivalent width
real*4 e_EW_1 (nr__1) ! (0.1nm) ?=- rms uncertainty on EW
character*1 l_A_Li_1 (nr__1) ! Limit flag on A(Li)
real*4 A_Li_1 (nr__1) ! ([Sun]) Lithium abundance (uncertainty=0.1dex)
integer*4 S_N_1 (nr__1) ! Signal-to-noise ratio
integer*4 Teff_1 (nr__1) ! (K) H{alpha}-based effective temperature
real*4 v_Fe_H__1 (nr__1) ! ([Sun]) ?=- Estimated metallicity (1)
character*1 n__Fe_H__1 (nr__1) ! [a] anomalous population SGB-a
* (table2 only, assumed metallicity)
real*4 e__Fe_H__1 (nr__1) ! ([Sun]) ?=- rms uncertainty on [Fe/H]
*Note (1): For three stars, no [Fe/H] was estimated. These stars were not
* plotted in the bottom panel of Fig. 3.
C=============================================================================
C Loading file 'table1.dat' ! Basic data for MS/SGB stars studied in this paper
C Format for file interpretation
1 format(
+ I6,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.1,1X,F3.1,
+ 1X,A1,F4.2,1X,I2,1X,I4,1X,F5.2,A1,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,91
read(1,'(A65)')ar__
read(ar__,1)
+ v_MBS2010_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),EW(i__),e_EW(i__),l_A_Li(i__),A_Li(i__),
+ S_N(i__),Teff(i__),v_Fe_H_(i__),n__Fe_H_(i__),e__Fe_H_(i__)
if (idig(ar__(33:36)).EQ.0) EW(i__) = rNULL__
if (idig(ar__(38:40)).EQ.0) e_EW(i__) = rNULL__
if (idig(ar__(56:60)).EQ.0) v_Fe_H_(i__) = rNULL__
if (idig(ar__(62:65)).EQ.0) e__Fe_H_(i__) = rNULL__
RAdeg(i__) = rNULL__
DEdeg(i__) = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ v_MBS2010_(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),EW(i__),e_EW(i__),l_A_Li(i__),A_Li(i__),
+ S_N(i__),Teff(i__),v_Fe_H_(i__),n__Fe_H_(i__),e__Fe_H_(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Basic data for SGB-a stars studied in this paper
C Format for file interpretation
2 format(
+ I6,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F4.1,1X,F3.1,
+ 1X,A1,F4.2,1X,I2,1X,I4,1X,F5.2,A1,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,10
read(1,'(A65)')ar__1
read(ar__1,2)
+ v_MBS2010__1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),EW_1(i__),e_EW_1(i__),
+ l_A_Li_1(i__),A_Li_1(i__),S_N_1(i__),Teff_1(i__),
+ v_Fe_H__1(i__),n__Fe_H__1(i__),e__Fe_H__1(i__)
if (idig(ar__1(33:36)).EQ.0) EW_1(i__) = rNULL__
if (idig(ar__1(38:40)).EQ.0) e_EW_1(i__) = rNULL__
if (idig(ar__1(56:60)).EQ.0) v_Fe_H__1(i__) = rNULL__
if (idig(ar__1(62:65)).EQ.0) e__Fe_H__1(i__) = rNULL__
RAdeg_1(i__) = rNULL__
DEdeg_1(i__) = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c ..............Just test output...........
write(6,2)
+ v_MBS2010__1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
+ DEd_1(i__),DEm_1(i__),DEs_1(i__),EW_1(i__),e_EW_1(i__),
+ l_A_Li_1(i__),A_Li_1(i__),S_N_1(i__),Teff_1(i__),
+ v_Fe_H__1(i__),n__Fe_H__1(i__),e__Fe_H__1(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end
C Locate position of first digit in string; or return 0
integer function idig(c)
character*(*) c
character*1 c1
integer lc,i
lc=len(c)
idig=0
do i=1,lc
if(c(i:i).ne.' ') go to 1
end do
1 if(i.gt.lc) return
c1=c(i:i)
if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1
if(i.gt.lc) return
c1=c(i:i)
if(c1.ge.'0'.and.c1.le.'9') idig=i
return
end