Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/419/1350 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-19 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/MNRAS/419/1350 Red giants abundances in 4 open clusters (Reddy+, 2012) *================================================================================ *Comprehensive abundance analysis of red giants in the open clusters *NGC 752, 1817, 2360 and 2506. * Reddy A.B.S., Giridhar S., Lambert D.L. * <Mon. Not. R. Astron. Soc., 419, 1350-1361 (2012)> * =2012MNRAS.419.1350R C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! The observed stars integer*4 nr__ parameter (nr__=14) ! Number of records character*64 ar__ ! Full-size record C J2000.0 position composed of: RAh RAm RAs DE- DEd DEm DEs real*8 RAdeg (nr__) ! (deg) Right Ascension J2000.0 real*8 DEdeg (nr__) ! (deg) Declination J2000.0 C ---------------------------------- ! (position vector(s) in degrees) character*8 Cluster (nr__) ! Cluster name integer*4 Star (nr__) ! Star number within the cluster integer*4 RAh (nr__) ! (h) Right ascension (J2000.0) integer*4 RAm (nr__) ! (min) Right ascension (J2000.0) real*4 RAs (nr__) ! (s) Right ascension (J2000.0) character*1 DE_ (nr__) ! Declination sign (J2000.0) integer*4 DEd (nr__) ! (deg) Declination (J2000.0) integer*4 DEm (nr__) ! (arcmin) Declination (J2000.0) real*4 DEs (nr__) ! (arcsec) Declination (J2000.0) real*4 Vmag (nr__) ! (mag) V magnitude real*4 B_V (nr__) ! (mag) B-V colour index real*4 HRV (nr__) ! (km/s) Heliocentric radial velocity real*4 e_HRV (nr__) ! (km/s) rms uncertainty on HRV integer*4 S_N (nr__) ! Signal-to-noise ration at 6000{AA} c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table6.dat' ! The line list for all program stars from each of the OCs presented in the paper integer*4 nr__1 parameter (nr__1=2430) ! Number of records character*45 ar__1 ! Full-size record character*8 Cluster_1 (nr__1) ! Cluster name integer*4 Star_1 (nr__1) ! Star number within the cluster real*8 lambda (nr__1) ! (0.1nm) Wavelength {lambda} in Angstroms real*4 Ion (nr__1) ! Species identification (1) real*4 LEP (nr__1) ! (eV) Lower Excitation potential of the transition real*4 log_gf (nr__1) ! ([-]) Log of the oscillator strength real*4 EW (nr__1) ! (0.1pm) Equivalent width in milli-Angstroms (2) *Note (1): The integer component of the species ID indicates the atomic * number, and the decimal component indicates the ionization state * (0=neutral, 1=singly ionized). *Note (2): The EW given for the synthesized line (MnI, CuI, BaII and EuII, * CeII and SmII) is the blend equivalent width. C============================================================================= C Loading file 'table2.dat' ! The observed stars C Format for file interpretation 1 format( + A8,1X,I4,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,F5.2, + 1X,F5.2,1X,F5.1,1X,F3.1,1X,I3) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,14 read(1,'(A64)')ar__ read(ar__,1) + Cluster(i__),Star(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),Vmag(i__),B_V(i__),HRV(i__), + e_HRV(i__),S_N(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) + Cluster(i__),Star(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__), + DEd(i__),DEm(i__),DEs(i__),Vmag(i__),B_V(i__),HRV(i__), + e_HRV(i__),S_N(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 'table6.dat' ! The line list for all program stars from each of * the OCs presented in the paper C Format for file interpretation 2 format(A8,1X,I4,1X,F7.2,1X,F5.1,1X,F5.2,1X,F5.2,1X,F5.1) C Effective file loading open(unit=1,status='old',file= +'table6.dat') write(6,*) '....Loading file: table6.dat' do i__=1,2430 read(1,'(A45)')ar__1 read(ar__1,2) + Cluster_1(i__),Star_1(i__),lambda(i__),Ion(i__),LEP(i__), + log_gf(i__),EW(i__) c ..............Just test output........... write(6,2) + Cluster_1(i__),Star_1(i__),lambda(i__),Ion(i__),LEP(i__), + log_gf(i__),EW(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end