Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/154/150 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 2024-Apr-18
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/AJ/154/150 Spectroscopy of RGB stars in {omega} Centauri (An+, 2017)
*================================================================================
*Medium-resolution spectroscopy of red giant branch stars in {omega} Centauri.
* An D., Lee Y.S., Jung J.In, Rey S.-C., Rhee J., Lee J.-W., Lee Y.-W.,
* Joe Y.H.
* <Astron. J., 154, 150 (2017)>
* =2017AJ....154..150A (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Spectroscopic Properties of Stars in {omega} Cen
integer*4 nr__
parameter (nr__=712) ! Number of records
character*108 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 Seq (nr__) ! [1/712] Sequential running star identifier
integer*4 RAh (nr__) ! (h) Hour of Right Ascension (J2000)
integer*4 RAm (nr__) ! (min) Minute of Right Ascension (J2000)
real*4 RAs (nr__) ! (s) Second of Right Ascension (J2000)
character*1 DE_ (nr__) ! Sign of the Declination (J2000)
integer*4 DEd (nr__) ! (deg) Degree of Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000)
real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000)
real*4 Vmag (nr__) ! (mag) [14.201/14.998] V band magnitude from
* Rey et al. 2004 (J/AJ/127/958)
real*4 B_V (nr__) ! (mag) [0.802/1.281] B-V color from Rey et al. 2004
* (J/AJ/127/958)
integer*4 Teff (nr__) ! (K) [4601/5410] Adjusted IRFM (Infrared Flux
* Method) effective temperature
integer*4 e_Teff (nr__) ! (K) [0/107]?=-99 Uncertainty in Teff
real*4 logg (nr__) ! ([cm/s2]) [0.5/4.04] Surface gravity
real*4 e_logg (nr__) ! ([cm/s2]) [0/1.49]?=-9.99 Uncertainty in logg
real*4 v_Fe_H_ (nr__) ! ([-]) [-2.28/0.21] Metallicity
real*4 e__Fe_H_ (nr__) ! ([-]) [0/1.54]?=-9.99 Uncertainty in [Fe/H]
real*4 v_Ca_Fe_ (nr__) ! ([-]) [-1.87/1.19] Calcium abundance
real*4 e__Ca_Fe_ (nr__) ! ([-]) [0.01/0.72]?=-9.99 Uncertainty in [Ca/Fe]
real*4 RV (nr__) ! (km/s) [-89.6/286.9]?=-999.9 Radial velocity
real*4 e_RV (nr__) ! (km/s) [0/60.4]?=-9.9 Uncertainty in RV
real*4 Fneighb (nr__) ! [0/0.98]?=-9.99 Fractional contribution of
* flux in B passband from neighboring stars
integer*4 Nobs (nr__) ! [1/3] Number of spectra with S/N>=52
character*1 Mem (nr__) ! [mx] Cluster membership (1)
*Note (1): Cluster membership, based on radial velocities and proper motions, is
* defined as follows:
* m = Cluster member;
* x = Non-member.
C=============================================================================
C Loading file 'table1.dat' ! Spectroscopic Properties of Stars in {omega} Cen
C Format for file interpretation
1 format(
+ I3,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F6.3,1X,F5.3,
+ 1X,I4,1X,I3,2X,F4.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,
+ 1X,F6.1,1X,F4.1,1X,F5.2,1X,I1,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,712
read(1,'(A108)')ar__
read(ar__,1)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),B_V(i__),Teff(i__),e_Teff(i__),
+ logg(i__),e_logg(i__),v_Fe_H_(i__),e__Fe_H_(i__),
+ v_Ca_Fe_(i__),e__Ca_Fe_(i__),RV(i__),e_RV(i__),Fneighb(i__),
+ Nobs(i__),Mem(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)
+ Seq(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),Vmag(i__),B_V(i__),Teff(i__),e_Teff(i__),
+ logg(i__),e_logg(i__),v_Fe_H_(i__),e__Fe_H_(i__),
+ v_Ca_Fe_(i__),e__Ca_Fe_(i__),RV(i__),e_RV(i__),Fneighb(i__),
+ Nobs(i__),Mem(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end