Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/805/65 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-Mar-28 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/ApJ/805/65 FLAMES observations of NGC 5128's globular clusters (Taylor+, 2015) *================================================================================ *Observational evidence for a dark side to NGC 5128's globular cluster system. * Taylor M.A., Puzia T.H., Gomez M., Woodley K.A. * <Astrophys. J., 805, 65 (2015)> * =2015ApJ...805...65T C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table1.dat' ! Star cluster observations integer*4 nr__ parameter (nr__=140) ! Number of records character*60 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 GC (nr__) ! [5/441] Cluster identifier (G1) integer*4 RAh (nr__) ! (h) [13] Hour of Right Ascension (J2000) integer*4 RAm (nr__) ! (min) [23/26] 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) [42/43] Degree of Declination (J2000) integer*4 DEm (nr__) ! (arcmin) Arcminute of Declination (J2000) real*4 DEs (nr__) ! (arcsec) Arcsecond of Declination (J2000) real*4 Rmag (nr__) ! (mag) [17/20.5] Apparent R band magnitude (1) real*4 Vmag (nr__) ! (mag) [16.8/20.7] Dereddened apparent V band * magnitude (2) real*4 e_Vmag (nr__) ! (mag) [0.01/0.2] Uncertainty in Vmag integer*4 Exp (nr__) ! (s) [1200/26400] Total integration time real*4 S_N (nr__) ! [0.2/11]?=-99 Signal-to-Noise ratio (3) *Note (1): Used for target acquisition. *Note (2): Or r'-band magnitudes. Most of our sample objects have apparent * V-band magnitudes provided in the Woodley et al. (2007, J/AJ/134/494) * catalog (see also references therein). Where V-band magnitudes are * not available, we list de-reddened r'-band magnitudes from * Sinnott et al. (2010, J/AJ/140/2101). See section 3.6. *Note (3): See Section 2.2 for a definition. A "-99." indicates the S/N * could not be estimated because no radial velocity was able * to be obtained from the literature or our data. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Star cluster kinematics integer*4 nr__1 parameter (nr__1=140) ! Number of records character*138 ar__1 ! Full-size record integer*4 GC_1 (nr__1) ! [5/441] Cluster identifier (G1) real*4 Rgc (nr__1) ! (arcmin) [1/21.5] Galacto-centric angular radius integer*4 RVlt (nr__1) ! (km/s) [146/890]?=-99 Literature radial velocity integer*4 e_RVlt (nr__1) ! (km/s) [1/202]?=-99 Uncertainty in RVlt integer*4 RV (nr__1) ! (km/s) [19/836]?=-99 Penalized pixel fitting technique * radial velocity real*4 e_RV (nr__1) ! (km/s) [0.3/31]?=-99 Uncertainty in RV real*4 sigma (nr__1) ! (km/s) [1/68]?=-99 Penalized pixel fitting technique * velocity dispersion {sigma} real*4 e_sigma (nr__1) ! (km/s) [0.3/52]?=-99 Uncertainty in sigma real*8 sig_ap (nr__1) ! (km/s) [3.6/68]?=-99 Model aperture corrected * velocity dispersion {sigma}_ap_ (4) real*8 E_sig_ap (nr__1) ! (km/s) ?=-99 Upper uncertainty in sig.ap real*8 e_sig_ap_1 (nr__1) ! (km/s) ?=-99 Lower uncertainty in sig.ap real*8 sig_gl (nr__1) ! (km/s) [3.5/62]?=-99 Global aperture corrected * velocity dispersion {sigma}_gl_ real*8 E_sig_gl (nr__1) ! (km/s) [0.02/18]?=-99 Upper uncertainty in sig.gl real*8 e_sig_gl_1 (nr__1) ! (km/s) [0.07/18]?=-99 Lower uncertainty in sig.gl real*4 sig_0 (nr__1) ! (km/s) [4/69.2]?=-99 Cluster core aperture corrected * velocity dispersion {sigma}_0_ real*8 E_sig_0 (nr__1) ! (km/s) ?=-99 Upper uncertainty in sig.0 real*4 e_sig_0_1 (nr__1) ! (km/s) ?=-99 Lower uncertainty in sig.0 real*4 sig_hl (nr__1) ! (km/s) [3.9/66]?=-99 Aperature corrected 2D projected * half-light radius velocity dispersion * {sigma}_1/2_ real*4 E_sig_hl (nr__1) ! (km/s) ?=-99 Upper uncertainty in sig.hl real*4 e_sig_hl_1 (nr__1) ! (km/s) ?=-99 Lower uncertainty in sig.hl integer*4 r_RVlt (nr__1) ! [1/5]?=-99 Reference code for RVlt (5) *Note (4): The model velocity dispersion corresponding to the FLAMES aperture. *Note (5): Reference as follows: * 1 = Woodley et al. (2010, J/AJ/139/1871); * 2 = Woodley et al. (2007, J/AJ/134/494), their mean; * 3 = Woodley et al. (2007, J/AJ/134/494), LDSS2; * 4 = Woodley et al. (2007, J/AJ/134/494), VIMOS; * 5 = Woodley et al. (2007, J/AJ/134/494), Hydra. c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! Star cluster structural parameters integer*4 nr__2 parameter (nr__2=140) ! Number of records character*125 ar__2 ! Full-size record integer*4 GC_2 (nr__2) ! [5/441] Cluster identifier (G1) real*8 Mhm (nr__2) ! (Msun) [0.03/7.5]?=-99 The 'half-mass' M_1/2_ (6) real*8 E_Mhm (nr__2) ! (Msun) ?=-99 Upper limit uncertainty in Mhm real*8 e_Mhm_1 (nr__2) ! (Msun) ?=-99 Lower limit uncertainty in Mhm real*8 Mdyn (nr__2) ! (Msun) [0.07/15.4]?=-99 Dynamical mass real*8 E_Mdyn (nr__2) ! (Msun) ?=-99 Upper limit uncertainty in Mdyn real*8 e_Mdyn_1 (nr__2) ! (Msun) ?=-99 Lower limit uncertainty in Mdyn real*4 M_Lhm (nr__2) ! (Msun/Lsun) [0.4/64.5]?=-99 The 'half-mass' * mass-to-light ratio real*4 E_M_Lhm (nr__2) ! (Msun/Lsun) ?=-99 Upper limit uncertainty in M/Lhm real*4 e_M_Lhm_1 (nr__2) ! (Msun/Lsun) ?=-99 Lower limit uncertainty in M/Lhm real*4 M_Ldyn (nr__2) ! (Msun/Lsun) [0.5/66.7]?=-99 Dynamic mass-to-light ratio real*4 E_M_Ldyn (nr__2) ! (Msun/Lsun) ?=-99 Upper limit uncertainty in M/Ldyn real*4 e_M_Ldyn_1 (nr__2) ! (Msun/Lsun) ?=-99 Lower limit uncertainty in M/Ldyn real*4 rh (nr__2) ! (pc) [0.2/23]?=-99 Half light radius real*4 e_rh (nr__2) ! (pc) ?=-99 Uncertainty in rh real*4 c (nr__2) ! [0.8/2.5]?=-99 Concentration parameter integer*4 r_rh (nr__2) ! ?=-99 Reference for rh (7) *Note (6): In other words the dynamical mass corresponding to that contained * within the 2D projected half-light radius. *Note (7): Reference as follows: * 1 = Gomez et al. (2015, in prep.); * 2 = Jordan et al. (2015, in prep.); * 3 = Harris et al. (2002AJ....124.1435H). C============================================================================= C Loading file 'table1.dat' ! Star cluster observations C Format for file interpretation 1 format( + I4,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F5.2,1X,F5.2, + 1X,F4.2,1X,I5,1X,F6.2) C Effective file loading open(unit=1,status='old',file= +'table1.dat') write(6,*) '....Loading file: table1.dat' do i__=1,140 read(1,'(A60)')ar__ read(ar__,1) + GC(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__), + DEs(i__),Rmag(i__),Vmag(i__),e_Vmag(i__),Exp(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) + GC(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__), + DEs(i__),Rmag(i__),Vmag(i__),e_Vmag(i__),Exp(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 'table2.dat' ! Star cluster kinematics C Format for file interpretation 2 format( + I4,1X,F5.2,1X,I3,1X,I3,1X,I3,1X,F6.2,1X,F6.2,1X,F6.2,1X,F7.3, + 1X,F7.3,1X,F7.3,1X,F7.3,1X,F7.3,1X,F7.3,1X,F6.2,1X,F7.3,1X, + F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,I3) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,140 read(1,'(A138)')ar__1 read(ar__1,2) + GC_1(i__),Rgc(i__),RVlt(i__),e_RVlt(i__),RV(i__),e_RV(i__), + sigma(i__),e_sigma(i__),sig_ap(i__),E_sig_ap(i__), + e_sig_ap_1(i__),sig_gl(i__),E_sig_gl(i__),e_sig_gl_1(i__), + sig_0(i__),E_sig_0(i__),e_sig_0_1(i__),sig_hl(i__), + E_sig_hl(i__),e_sig_hl_1(i__),r_RVlt(i__) c ..............Just test output........... write(6,2) + GC_1(i__),Rgc(i__),RVlt(i__),e_RVlt(i__),RV(i__),e_RV(i__), + sigma(i__),e_sigma(i__),sig_ap(i__),E_sig_ap(i__), + e_sig_ap_1(i__),sig_gl(i__),E_sig_gl(i__),e_sig_gl_1(i__), + sig_0(i__),E_sig_0(i__),e_sig_0_1(i__),sig_hl(i__), + E_sig_hl(i__),e_sig_hl_1(i__),r_RVlt(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table3.dat' ! Star cluster structural parameters C Format for file interpretation 3 format( + I4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F6.2,1X, + F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2,1X,F6.2, + 1X,I3) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,140 read(1,'(A125)')ar__2 read(ar__2,3) + GC_2(i__),Mhm(i__),E_Mhm(i__),e_Mhm_1(i__),Mdyn(i__), + E_Mdyn(i__),e_Mdyn_1(i__),M_Lhm(i__),E_M_Lhm(i__), + e_M_Lhm_1(i__),M_Ldyn(i__),E_M_Ldyn(i__),e_M_Ldyn_1(i__), + rh(i__),e_rh(i__),c(i__),r_rh(i__) c ..............Just test output........... write(6,3) + GC_2(i__),Mhm(i__),E_Mhm(i__),e_Mhm_1(i__),Mdyn(i__), + E_Mdyn(i__),e_Mdyn_1(i__),M_Lhm(i__),E_M_Lhm(i__), + e_M_Lhm_1(i__),M_Ldyn(i__),E_M_Ldyn(i__),e_M_Ldyn_1(i__), + rh(i__),e_rh(i__),c(i__),r_rh(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end