Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/486/177 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-Oct-14
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/486/177 Bulge field stars from FLAMES-GIRAFFE spectra (Zoccali+, 2008)
*================================================================================
*The metal content of bulge field stars from FLAMES-GIRAFFE spectra.
*I. Stellar parameters and iron abundances.
* Zoccali M., Hill V., Lecureur A., Barbuy B., Renzini A., Minniti D.,
* Gomez A., Ortolani S.
* <Astron. Astrophys., 486, 177-189 (2008)>
* =2008A&A...486..177Z
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Stellar parameters and iron abundance of all
the program stars
integer*4 nr__
parameter (nr__=521) ! Number of records
character*87 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)
character*1 Fld (nr__) ! [ABC] Field with A = Baade windows,
* B = Field at b=-6{deg},
* C = Field at b=-12{deg}
integer*4 QF (nr__) ! [0/2] Subjective quality factor (1)
integer*4 ID (nr__) ! [2/135] Identification number (not unique!)
character*8 OGLE (nr__) ! OGLE identification number (2)
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) [0/60] Declination (J2000)
real*4 Vmag (nr__) ! (mag) V magnitude
real*4 V_I (nr__) ! (mag) V-I colour index
real*4 logg (nr__) ! ([cm/s2]) Surface gravity
real*4 Vt (nr__) ! (km/s) Microturbulence velocity
integer*4 Teff (nr__) ! (K) Effective temperature
real*4 v_Fe_H_ (nr__) ! ([Sun]) Metallicity
real*4 e__Fe_H_ (nr__) ! ([Sun]) Line-to-line dispersion around the mean [Fe/H]
character*8 Cluster (nr__) ! Cluster name
*Note (1): QF is a subjective quality factor, classifying stars into good
* (0), bad (2) and intermediate (1), according to how unique/degenerate
* the convergence into the final model atmosphere proceeded.
*Note (2): For field A, stars identified as OGLE BUL-SC45 NNNNNN in Simbad,
* from Udalski et al., 2002, Cat. <J/AcA/52/217>
C=============================================================================
C Loading file 'table3.dat' ! Stellar parameters and iron abundance of all
* the program stars
C Format for file interpretation
1 format(
+ A1,1X,I1,1X,I3,1X,A8,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,
+ F5.2,1X,F5.2,1X,F5.3,1X,F4.2,1X,F3.1,1X,I4,1X,F5.2,1X,F4.2,1X,
+ A8)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,521
read(1,'(A87)')ar__
read(ar__,1)
+ Fld(i__),QF(i__),ID(i__),OGLE(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Vmag(i__),V_I(i__),
+ logg(i__),Vt(i__),Teff(i__),v_Fe_H_(i__),e__Fe_H_(i__),
+ Cluster(i__)
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)
+ Fld(i__),QF(i__),ID(i__),OGLE(i__),RAh(i__),RAm(i__),RAs(i__),
+ DE_(i__),DEd(i__),DEm(i__),DEs(i__),Vmag(i__),V_I(i__),
+ logg(i__),Vt(i__),Teff(i__),v_Fe_H_(i__),e__Fe_H_(i__),
+ Cluster(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end