FORTRAN Generation
(/./home/cats/J/AJ/152/208)

Conversion of standardized ReadMe file for file /./home/cats/J/AJ/152/208 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-May-10
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/152/208      Ages and metallicities for M31 star clusters      (Fan+, 2016)
*================================================================================
*Lick indices and spectral energy distribution analysis based on an M31 star
*cluster sample: comparisons of methods and models.
*    Fan Z., de Grijs R., Chen B., Jiang L., Bian F., Li Z.
*   <Astron. J., 152, 208-208 (2016)>
*   =2016AJ....152..208F    (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table1.dat'	! Observations of our sample globular clusters

      integer*4 nr__
      parameter (nr__=22)	! Number of records
      character*66 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*10  Name       (nr__) ! Globular cluster identification
      integer*4     RAh        (nr__) ! (h) Hour of Right Ascension (J2000) (1)
      integer*4     RAm        (nr__) ! (min) Minute of Right Ascension (J2000) (1)
      real*4        RAs        (nr__) ! (s) Second of Right Ascension (J2000) (1)
      character*1   DE_        (nr__) ! Sign of the Declination (1)
      integer*4     DEd        (nr__) ! (deg) Degree of Declination (J2000) (1)
      integer*4     DEm        (nr__) ! (arcmin) Arcminute of Declination (J2000) (1)
      real*4        DEs        (nr__) ! (arcsec) Arcsecond of Declination (J2000) (1)
      real*4        Rp         (nr__) ! (kpc) Projected radius from the galaxy center
*                                   (r_p_) (1)
      real*4        Vmag       (nr__) ! (mag) V-band magnitude (1)
      integer*4     Exp        (nr__) ! (s) Exposure time of individual observation
      integer*4     Nexp       (nr__) ! ? Number of exposures
      character*11  Date       (nr__) ! ("Y:M:D") Date of observation
*Note (1): The coordinates, r_p_ and V-band magnitudes were taken from the
*     Revised Bologna Catalog (RBC) v.5. (Galleti et al. 2012, Cat. V/143).

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table2.dat'	! Radial velocities, V_r_, of our sample globular
                                  clusters as well as previously published
                                  measurements

      integer*4 nr__1
      parameter (nr__1=22)	! Number of records
      character*39 ar__1  	! Full-size record

      character*10  Name_1     (nr__1) ! Globular cluster identification
      character*1   f_Name     (nr__1) ! [1a] Flag on Name (2)
      integer*4     RV1        (nr__1) ! (km/s) [-673/45] Radial velocity fitted with ULySS
*                                 based on the model of Vazdekis et al. 2010
*                                 (Cat. J/MNRAS/404/1639) (3)
      integer*4     e_RV1      (nr__1) ! (km/s) [1/120] Uncertainty in RV1 (3)
      integer*4     RV2        (nr__1) ! (km/s) [-681/54] Radial velocity fitted with ULySS
*                                 based on the PEGASE-HR model (3)
      integer*4     e_RV2      (nr__1) ! (km/s) [1/60] Uncertainty in RV2 (3)
      integer*4     RV3        (nr__1) ! (km/s) [-561/33]? Radial velocity from the Revised
*                                 Bologna Catalog (RBC) v.5. (Galleti et al.
*                                 2012, Cat. V/143)
      integer*4     e_RV3      (nr__1) ! (km/s) [1/47]? Uncertainty in RV3
      character*1   f_RV3      (nr__1) ! [a] Flag 'a' on RV3 indicates that the RBC
*                                 radial velocity was modified in -188+/-26km/s
*                                 at CDS (4)
*Note (2): Flag defined as follows:
*     1 = This flag was not explained in the text;
*     a = In Table2, the repeated object G339-BA30 (in the paper) was modified in
*         B339-G077 at CDS.
*Note (3): Fitted with Universite de Lyon Spectroscopic analysis Software (ULySS;
*     http://ulyss.univ-lyon1.fr/; see Koleva et al. 2009A&A...501.1269K,
*     Chen et al. 2016, Cat. J/AJ/152/45).
*Note (4): In Table2 of the paper, the RBC radial velocity of G339-BA30 was
*     33+/-30km/s. As we modified G339-BA30 in B339-G077 at CDS, we changed the
*     RBC radial velocity in -188+/-26km/s (from the Revised Bologna Catalog v.5.
*     of Galleti et al. 2012, Cat. V/143).

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table3.dat'	! Ages and metallicities derived from the Lick
                                  absorption-line indices fitted with ULySS

      integer*4 nr__2
      parameter (nr__2=22)	! Number of records
      character*62 ar__2  	! Full-size record

      character*10  Name_2     (nr__2) ! Globular cluster identification
      real*4        logAge1    (nr__2) ! (yr) [9.3/10.25] Log of age for the Vazdekis et
*                                    al. 2010 (Cat. J/MNRAS/404/1639) SSP
*                                    model (5)
      real*4        e_logAge1  (nr__2) ! (yr) [0/0.07] Error in logAge1 (5)
      real*4        logAge2    (nr__2) ! (yr) [9.4/10.4] Log of age for the PEGASE-HR SSP
*                                    model (6)
      real*4        e_logAge2  (nr__2) ! (yr) [0/0.042] Error in logAge2 (6)
      real*4        v_Fe_H_1   (nr__2) ! ([Sun]) [-2.32/-0.35] Metallicity for the Vazdekis et
*                                    al. 2010 (Cat. J/MNRAS/404/1639) SSP
*                                    model (5)
      real*4        e__Fe_H_1  (nr__2) ! ([Sun]) [0.01/0.04] Error in [Fe/H]1 (5)
      real*4        v_Fe_H_2   (nr__2) ! ([Sun]) [-2.3/-0.4] Metallicity for the PEGASE-HR SSP
*                                    model (6)
      real*4        e__Fe_H_2  (nr__2) ! ([Sun]) [0.01/0.03] Error in [Fe/H]2 (6)
*Note (5): Logarithmic age and metallicity derived based on the Lick
*     absorption-line index and fitted with Universite de Lyon Spectroscopic
*     analysis Software (ULySS; http://ulyss.univ-lyon1.fr/; see Koleva et al.
*     2009A&A...501.1269K, Chen et al. 2016, Cat. J/AJ/152/45), for the Vazdekis
*     et al. 2010 (Cat. J/MNRAS/404/1639) Simple Stellar Population (SSP) model.
*Note (6): Logarithmic age and metallicity derived based on the Lick
*     absorption-line index and fitted with ULySS, for PEGASE-HR Simple Stellar
*     Population (SSP) model (provided by Le Borgne et al. 2004A&A...425..881L).

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table4.dat'	! Ages and metallicities derived from the Lick
                                  absorption-line indices fitted with EZ_Ages

      integer*4 nr__3
      parameter (nr__3=22)	! Number of records
      character*34 ar__3  	! Full-size record

      character*10  Name_3     (nr__3) ! Globular cluster identification
      real*4        logAge3    (nr__3) ! (Gyr) [2/12.21]?=99.99 Age derived with EZ_Ages (7)
      real*4        v_Fe_H_3   (nr__3) ! ([Sun]) [-1.12/-0.18]?=99.99 Metallicity derived with
*                                EZ_Ages (7)
      real*4        v_Fe_H_4   (nr__3) ! ([Sun]) [-2.25/-0.35] Metallicity derived from [MgFe] (8)
      real*4        v_Fe_H_5   (nr__3) ! ([Sun]) [-2.95/-0.39] Metallicity derived from <Fe> (9)
*Note (7): Ages and metallicities derived from the Lick absorption-line indices
*     fitted with EZ_Ages.
*Note (8):
*     [MgFe]=(Mgb*<Fe>)^1/2^, where <Fe> =(Fe5270+Fe5335)/2.
*     Thus, the metallicity can be calculated following Galleti et al. 2009
*     (Cat. J/A+A/508/1285), using
*     [Fe/H]_[MgFe]_=-2.563+1.119[MgFe]-0.106[MgFe]^2^+/-0.15dex(rms) Eq. (1).
*Note (9): Derived from <Fe> =(Fe5270+Fe5335)/2 following Caldwell et al. 2011
*     (Cat. J/AJ/141/61).

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table5.dat'	! Ages and metallicities derived from the Lick
                                  absorption-line indices fitted with the
                                  Thomas et al. 2011MNRAS.412.2183T models

      integer*4 nr__4
      parameter (nr__4=22)	! Number of records
      character*75 ar__4  	! Full-size record

      character*10  Name_4     (nr__4) ! Globular cluster identification
      real*4        logAge4    (nr__4) ! (yr) [8/10.2] Log of age derived from the Lick
*                                   absorption-line index fitted with the Thomas
*                                   et al. 2011MNRAS.412.2183T models (10)
      real*4        e_logAge4  (nr__4) ! (yr) [0/0.22] Negative error in logAge4
      real*4        E_logAge4_1(nr__4) ! (yr) [0/0.19] Positive error in logAge4
      real*4        v_Z_H_     (nr__4) ! ([Sun]) [-2.2/-0.29] Metallicity derived from the Lick
*                                   absorption-line index fitted with the Thomas
*                                   et al. 2011MNRAS.412.2183T models (10)
      real*4        e__Z_H_    (nr__4) ! ([Sun]) [0.09/0.47] Negative error in [Z/H]
      real*4        E__Z_H__1  (nr__4) ! ([Sun]) [0.1/0.75] Positive error in [Z/H]
      real*4        v_a_Fe_    (nr__4) ! ([Sun]) [-0.3/0.5] [{alpha}/Fe] ratio derived from the
*                                   Lick absorption-line index fitted with the
*                                   Thomas et al. 2011MNRAS.412.2183T models (10)
      real*4        e__a_Fe_   (nr__4) ! ([Sun]) [0/0.8] Negative error in [a/Fe]
      real*4        E__a_Fe__1 (nr__4) ! ([Sun]) [0/0.8] Positive error in [a/Fe]
*Note (10): For the evolutionary tracks of Cassisi et al. 1997A&A...317..108C and
*     the Padova models of Thomas et al. 2011MNRAS.412.2183T.

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table6.dat'	! Ages and metallicities derived from the Lick
                                  absorption-line indices fitted with the GALEV
                                  models

      integer*4 nr__5
      parameter (nr__5=22)	! Number of records
      character*52 ar__5  	! Full-size record

      character*10  Name_5     (nr__5) ! Globular cluster identification
      real*4        logAge5    (nr__5) ! (yr) [6.6/10.2] Log of age derived from the Lick
*                                  absorption-line index fitted with the GALEV
*                                  models (11)
      real*4        e_logAge5  (nr__5) ! (yr) [0/0.315] Negative error in logAge5
      real*4        E_logAge5_1(nr__5) ! (yr) [0/0.85] Positive error in logAge5
      real*4        v_Fe_H_6   (nr__5) ! ([Sun]) [-2.2/0.24] Metallicity derived from the Lick
*                                  absorption-line index fitted with the GALEV
*                                  models (11)
      real*4        e__Fe_H_6  (nr__5) ! ([Sun]) [0.075/0.76] Negative error in [Fe/H]
      real*4        E__Fe_H_6_1(nr__5) ! ([Sun]) [0.001/1.5] Positive error in [Fe/H]
*Note (11): Fitted with the Galaxy Evolutionary Synthesis Models (GALEV; Lilly &
*     Fritze-v. Alvensleben 2006A&A...457..467L; Kotulla et al.
*     2009MNRAS.396..462K; see also Section 4.3 for additional details about the
*     GALEV models).

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table7.dat'	! Lick/IDS index {chi}_min_^2^ fit results using
                                  Bruzual & Charlot 2003MNRAS.344.1000B models

      integer*4 nr__6
      parameter (nr__6=88)	! Number of records
      character*142 ar__6  	! Full-size record

      character*1   IMF        (nr__6) ! Initial Mass Function (C=Chabrier, or
*                                   S=Salpeter) (1)
      character*3   SET        (nr__6) ! Stellar Evolutionary Tracks (P00 or P94) (2)
      character*10  Name_6     (nr__6) ! Globular cluster identification
      real*4        logAge6    (nr__6) ! (yr) [6.4/10.1] Lick/IDS log of age (3)
      real*4        e_logAge6  (nr__6) ! (yr) [0.02/0.45] Negative error in logAge6
      real*4        E_logAge6_1(nr__6) ! (yr) [0.024/0.44] Positive error in logAge6
      real*4        v_Fe_H_7   (nr__6) ! ([Sun]) [-2.25/0.28] Lick/IDS metallicity (3)
      real*4        e__Fe_H_7  (nr__6) ! ([Sun]) [0/0.5] Negative error in [Fe/H]7
      real*4        E__Fe_H_7_1(nr__6) ! ([Sun]) [0.048/0.55] Positive error in [Fe/H]7
      real*4        logAge7    (nr__6) ! (yr) [8.9/10.2] SED log of age (4)
      real*4        e_logAge7  (nr__6) ! (yr) [0.004/0.62] Negative error in logAge7
      real*4        E_logAge7_1(nr__6) ! (yr) [0/0.63] Positive error in logAge7
      real*4        v_Fe_H_8   (nr__6) ! ([Sun]) [-2.25/0.56] SED metallicity (4)
      real*4        e__Fe_H_8  (nr__6) ! ([Sun]) [0/0.74] Negative error in [Fe/H]8
      real*4        E__Fe_H_8_1(nr__6) ! ([Sun]) [0/0.86] Positive error in [Fe/H]8
      real*4        logAge8    (nr__6) ! (yr) [6.6/10.14] Log of age from both fits (5)
      real*4        e_logAge8  (nr__6) ! (yr) [0.01/0.7] Negative error in logAge8
      real*4        E_logAge8_1(nr__6) ! (yr) [0/3.5] Positive error in logAge8
      real*4        v_Fe_H_9   (nr__6) ! ([Sun]) [-2.25/-0.17] Metallicity from both fits (5)
      real*4        e__Fe_H_9  (nr__6) ! ([Sun]) [0/0.57] Negative error in [Fe/H]9
      real*4        E__Fe_H_9_1(nr__6) ! ([Sun]) [0.06/0.73] Positive error in [Fe/H]9
*Note (1): Source of the stellar initial mass function:
*     S = Stellar initial mass function (IMF) of Salpeter 1955ApJ...121..161S;
*     C = Stellar initial mass function (IMF) of Chabrier 2003PASP..115..763C.
*Note (2): Source of stellar evolutionary tracks:
*     P00 = 2000 Padova stellar evolutionary tracks;
*     P94 = 1994 Padova stellar evolutionary tracks.
*Note (3): Derived only from Lick/IDS absorption-line index fits.
*Note (4): Derived, only based on Spectral Energy Distribution (SED) fitting.
*Note (5): Derived from both the Lick/IDS absorption indices and the SED fits.

C=============================================================================

C  Loading file 'table1.dat'	! Observations of our sample globular clusters

C  Format for file interpretation

    1 format(
     +  A10,1X,I2,1X,I2,1X,F6.3,1X,A1,I2,1X,I2,1X,F5.2,1X,F5.2,1X,
     +  F5.2,1X,I3,1X,I1,1X,A11)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,22
        read(1,'(A66)')ar__
        read(ar__,1)
     +  Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
     +  DEm(i__),DEs(i__),Rp(i__),Vmag(i__),Exp(i__),Nexp(i__),
     +  Date(i__)
        if(ar__(54:54) .EQ. '') Nexp(i__) = iNULL__
        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)
     +  Name(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
     +  DEm(i__),DEs(i__),Rp(i__),Vmag(i__),Exp(i__),Nexp(i__),
     +  Date(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'	! Radial velocities, V_r_, of our sample globular
*                                  clusters as well as previously published
*                                  measurements

C  Format for file interpretation

    2 format(A10,1X,A1,1X,I4,1X,I3,1X,I4,1X,I2,1X,I4,1X,I2,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,22
        read(1,'(A39)')ar__1
        read(ar__1,2)
     +  Name_1(i__),f_Name(i__),RV1(i__),e_RV1(i__),RV2(i__),
     +  e_RV2(i__),RV3(i__),e_RV3(i__),f_RV3(i__)
        if(ar__1(31:34) .EQ. '') RV3(i__) = iNULL__
        if(ar__1(36:37) .EQ. '') e_RV3(i__) = iNULL__
c    ..............Just test output...........
        write(6,2)
     +  Name_1(i__),f_Name(i__),RV1(i__),e_RV1(i__),RV2(i__),
     +  e_RV2(i__),RV3(i__),e_RV3(i__),f_RV3(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================

C  Loading file 'table3.dat'	! Ages and metallicities derived from the Lick
*                                  absorption-line indices fitted with ULySS

C  Format for file interpretation

    3 format(
     +  A10,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,
     +  1X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,22
        read(1,'(A62)')ar__2
        read(ar__2,3)
     +  Name_2(i__),logAge1(i__),e_logAge1(i__),logAge2(i__),
     +  e_logAge2(i__),v_Fe_H_1(i__),e__Fe_H_1(i__),v_Fe_H_2(i__),
     +  e__Fe_H_2(i__)
c    ..............Just test output...........
        write(6,3)
     +  Name_2(i__),logAge1(i__),e_logAge1(i__),logAge2(i__),
     +  e_logAge2(i__),v_Fe_H_1(i__),e__Fe_H_1(i__),v_Fe_H_2(i__),
     +  e__Fe_H_2(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================

C  Loading file 'table4.dat'	! Ages and metallicities derived from the Lick
*                                  absorption-line indices fitted with EZ_Ages

C  Format for file interpretation

    4 format(A10,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table4.dat')
      write(6,*) '....Loading file: table4.dat'
      do i__=1,22
        read(1,'(A34)')ar__3
        read(ar__3,4)
     +  Name_3(i__),logAge3(i__),v_Fe_H_3(i__),v_Fe_H_4(i__),
     +  v_Fe_H_5(i__)
c    ..............Just test output...........
        write(6,4)
     +  Name_3(i__),logAge3(i__),v_Fe_H_3(i__),v_Fe_H_4(i__),
     +  v_Fe_H_5(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================

C  Loading file 'table5.dat'	! Ages and metallicities derived from the Lick
*                                  absorption-line indices fitted with the
*                                  Thomas et al. 2011MNRAS.412.2183T models

C  Format for file interpretation

    5 format(
     +  A10,3X,F6.3,2X,F5.3,2X,F5.3,1X,F6.3,2X,F5.3,2X,F5.3,1X,F6.3,
     +  2X,F5.3,2X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table5.dat')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,22
        read(1,'(A75)')ar__4
        read(ar__4,5)
     +  Name_4(i__),logAge4(i__),e_logAge4(i__),E_logAge4_1(i__),
     +  v_Z_H_(i__),e__Z_H_(i__),E__Z_H__1(i__),v_a_Fe_(i__),
     +  e__a_Fe_(i__),E__a_Fe__1(i__)
c    ..............Just test output...........
        write(6,5)
     +  Name_4(i__),logAge4(i__),e_logAge4(i__),E_logAge4_1(i__),
     +  v_Z_H_(i__),e__Z_H_(i__),E__Z_H__1(i__),v_a_Fe_(i__),
     +  e__a_Fe_(i__),E__a_Fe__1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================

C  Loading file 'table6.dat'	! Ages and metallicities derived from the Lick
*                                  absorption-line indices fitted with the GALEV
*                                  models

C  Format for file interpretation

    6 format(A10,1X,F6.3,2X,F5.3,2X,F5.3,1X,F6.3,2X,F5.3,2X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table6.dat')
      write(6,*) '....Loading file: table6.dat'
      do i__=1,22
        read(1,'(A52)')ar__5
        read(ar__5,6)
     +  Name_5(i__),logAge5(i__),e_logAge5(i__),E_logAge5_1(i__),
     +  v_Fe_H_6(i__),e__Fe_H_6(i__),E__Fe_H_6_1(i__)
c    ..............Just test output...........
        write(6,6)
     +  Name_5(i__),logAge5(i__),e_logAge5(i__),E_logAge5_1(i__),
     +  v_Fe_H_6(i__),e__Fe_H_6(i__),E__Fe_H_6_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================

C  Loading file 'table7.dat'	! Lick/IDS index {chi}_min_^2^ fit results using
*                                  Bruzual & Charlot 2003MNRAS.344.1000B models

C  Format for file interpretation

    7 format(
     +  A1,1X,A3,1X,A10,1X,F6.3,2X,F5.3,2X,F5.3,1X,F6.3,2X,F5.3,2X,
     +  F5.3,1X,F6.3,2X,F5.3,2X,F5.3,1X,F6.3,2X,F5.3,2X,F5.3,1X,F6.3,
     +  2X,F5.3,2X,F5.3,1X,F6.3,2X,F5.3,2X,F5.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table7.dat')
      write(6,*) '....Loading file: table7.dat'
      do i__=1,88
        read(1,'(A142)')ar__6
        read(ar__6,7)
     +  IMF(i__),SET(i__),Name_6(i__),logAge6(i__),e_logAge6(i__),
     +  E_logAge6_1(i__),v_Fe_H_7(i__),e__Fe_H_7(i__),
     +  E__Fe_H_7_1(i__),logAge7(i__),e_logAge7(i__),E_logAge7_1(i__),
     +  v_Fe_H_8(i__),e__Fe_H_8(i__),E__Fe_H_8_1(i__),logAge8(i__),
     +  e_logAge8(i__),E_logAge8_1(i__),v_Fe_H_9(i__),e__Fe_H_9(i__),
     +  E__Fe_H_9_1(i__)
c    ..............Just test output...........
        write(6,7)
     +  IMF(i__),SET(i__),Name_6(i__),logAge6(i__),e_logAge6(i__),
     +  E_logAge6_1(i__),v_Fe_H_7(i__),e__Fe_H_7(i__),
     +  E__Fe_H_7_1(i__),logAge7(i__),e_logAge7(i__),E_logAge7_1(i__),
     +  v_Fe_H_8(i__),e__Fe_H_8(i__),E__Fe_H_8_1(i__),logAge8(i__),
     +  e_logAge8(i__),E_logAge8_1(i__),v_Fe_H_9(i__),e__Fe_H_9(i__),
     +  E__Fe_H_9_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================
      stop
      end