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