Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/356/238 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/A+A/356/238 Atmospheric parameters in metal-poor stars. III. (Carretta+ 2000) *================================================================================ *Abundances of light elements in metal-poor stars. III. Data analysis and results * Carretta E., Gratton R.G., Sneden C. * <Astron. Astrophys. 356, 238 (2000)> * =2000A&A...356..238C C============================================================================= C Internal variables integer*4 i__ c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table2.dat' ! Equivalent widths for O, Na lines in the 19 program stars and the Sun integer*4 nr__ parameter (nr__=20) ! Number of records character*77 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 HD (nr__) ! HD designation (or Sun) integer*4 RAh (nr__) ! (h) ? Right ascension (J2000) (1) integer*4 RAm (nr__) ! (min) ? Right ascension (J2000) (1) real*4 RAs (nr__) ! (s) ? Right ascension (J2000) (1) character*1 DE_ (nr__) ! ? Declination sign (J2000) (1) integer*4 DEd (nr__) ! (deg) ? Declination (J2000) (1) integer*4 DEm (nr__) ! (arcmin) ? Declination (J2000) (1) integer*4 DEs (nr__) ! (arcsec) ? Declination (J2000) (1) real*4 EWOI6300 (nr__) ! (0.1nm) Equivalent widths for forbidden O I line * at 6300 Angstrom real*4 EWOI7771 (nr__) ! (0.1nm) Equivalent widths for permitted O I line * at 7771 Angstrom real*4 EWOI7772 (nr__) ! (0.1nm) Equivalent widths for permitted O I line * at 7772 Angstrom real*4 EWOI7774 (nr__) ! (0.1nm) Equivalent widths for permitted O I line * at 7774 Angstrom real*4 EWNaI4751 (nr__) ! (0.1nm) Equivalent widths for Na I line * at 4751 Angstrom real*4 EWNaI5682 (nr__) ! (0.1nm) Equivalent widths for Na I line * at 5682 Angstrom real*4 EWNaI5688 (nr__) ! (0.1nm) Equivalent widths for Na I line * at 5688 Angstrom real*4 EWNaI6154 (nr__) ! (0.1nm) Equivalent widths for Na I line * at 6154 Angstrom *Note (1): Positions from Simbad database c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table3.dat' ! CNO abundances and C12/C13 ratios for the 19 program stars integer*4 nr__1 parameter (nr__1=19) ! Number of records character*84 ar__1 ! Full-size record character*10 HD_1 (nr__1) ! HD designation real*4 v_Fe_H_ (nr__1) ! ([Sun]) Relative abundance of [Fe/H] real*4 v_C_Fe_CH (nr__1) ! ([Sun]) Relative abundance of [C/Fe] from CH real*4 v_C_Fe_C2 (nr__1) ! ([Sun]) ? Relative abundance of [C/Fe] from C_2_ real*4 v_N_Fe_b (nr__1) ! ([Sun]) ? Relative abundance of [N/Fe] from * CN blue system real*4 v_N_Fe_r (nr__1) ! ([Sun]) ? Relative abundance of [N/Fe] from CN * red system real*4 v_N_Fe_ (nr__1) ! ([Sun]) ? Mean relative abundance of [N/Fe] real*4 v_O_Fe_1 (nr__1) ! ([Sun]) ? Relative abundance of [O/Fe] from [O I] real*4 v_O_Fe_2 (nr__1) ! ([Sun]) ? Relative abundance of [O/Fe] from O I real*4 v_O_Fe_ (nr__1) ! ([Sun]) Mean relative abundance of [O/Fe] character*1 l_C12_C13 (nr__1) ! Limit flag on C12/C13 integer*4 C12_C13 (nr__1) ! ? Isotopic ratio C12/C13 real*4 v__C_N__Fe_(nr__1) ! ([Sun]) Relative abundance of [(C+N)/Fe] real*4 v_C_N_ (nr__1) ! ([Sun]) ? Relative abundance of [C/N] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table4.dat' ! Reanalysis of data by Tomkin et al. (1992AJ....104.1568T) integer*4 nr__2 parameter (nr__2=34) ! Number of records character*56 ar__2 ! Full-size record character*10 Name (nr__2) ! HD/BD designation integer*4 Teff (nr__2) ! (K) Effective temperature (K) real*4 logg (nr__2) ! ([cm/s2]) Suface gravity real*4 logLum (nr__2) ! ([solLum]) Logaritm of the luminosity real*4 v_Fe_H__1 (nr__2) ! ([Sun]) Metallicity real*4 xi (nr__2) ! (km/s) Microturbulent velocity character*1 l__C_Fe_ (nr__2) ! Limit flag on [C/Fe] real*4 v_C_Fe_ (nr__2) ! ([Sun]) ? Relative abundance [C/Fe] real*4 v_O_Fe_l (nr__2) ! ([Sun]) ? LTE relative abundance [O/Fe] real*4 v_O_Fe_n (nr__2) ! ([Sun]) ? NLTE relative abundance [O/Fe] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table5.dat' ! Reanalysis of data by Sneden et al. (1991AJ....102.2001S) and Kraft et al. (1992AJ....104..645K) integer*4 nr__3 parameter (nr__3=27) ! Number of records character*56 ar__3 ! Full-size record character*10 Name_1 (nr__3) ! HD/DM designation integer*4 Teff_1 (nr__3) ! (K) Effective temperature real*4 logg_1 (nr__3) ! ([cm/s2]) Surface gravity real*4 logLum_1 (nr__3) ! ([solLum]) Logaritm of the luminosity real*4 v_Fe_H__2 (nr__3) ! ([Sun]) Metallicity real*4 xi_1 (nr__3) ! (km/s) Microturbulent velocity real*4 v_O_Fe__1 (nr__3) ! ([Sun]) Relative abundance [O/Fe] from [O I] real*4 v_Na_Fe_l (nr__3) ! ([Sun]) ? LTE relative abundance [Na/Fe] real*4 v_Na_Fe_n (nr__3) ! ([Sun]) ? NLTE relative abundance [Na/Fe] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table6.dat' ! Reanalysis of data by Edvardsson et al. (1993, Cat. <J/A+A/275/101>) integer*4 nr__4 parameter (nr__4=187) ! Number of records character*86 ar__4 ! Full-size record character*10 Name_2 (nr__4) ! BS/HD designation integer*4 Teff_2 (nr__4) ! (K) Effective temperature real*4 logg_2 (nr__4) ! ([cm/s2]) Surface gravity real*4 logLum_2 (nr__4) ! ([solLum]) Logaritm of the luminosity real*4 v_Fe_H__3 (nr__4) ! ([Sun]) Matallicity real*4 xi_2 (nr__4) ! (km/s) Microturbulent velocity real*4 v_C_Fe_1 (nr__4) ! ([Sun]) ? Relative intensity [C/Fe] from C I character*1 l__C_Fe_2 (nr__4) ! Limit flag on [C/Fe]2 real*4 v_C_Fe_2 (nr__4) ! ([Sun]) ? Relative intensity [C/Fe] from [C I] real*4 v_O_Fe_1_1 (nr__4) ! ([Sun]) ? Relative intensity [O/Fe] from O I LTE real*4 v_O_Fe_2_1 (nr__4) ! ([Sun]) ? Relative intensity [O/Fe] from O I NLTE real*4 v_O_Fe_3 (nr__4) ! ([Sun]) ? Relative intensity [O/Fe] from [O I] real*4 v_Na_Fe_l_1(nr__4) ! ([Sun]) ? LTE relative intensity [Na/Fe] real*4 v_Na_Fe_n_1(nr__4) ! ([Sun]) ? NLTE relative intensity [Na/Fe] real*4 v_Mg_Fe_ (nr__4) ! ([Sun]) ? LTE relative intensity [Mg/Fe] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table7.dat' ! Reanalysis of data by Zhao & Magain (1990A&A...238..242Z) integer*4 nr__5 parameter (nr__5=20) ! Number of records character*60 ar__5 ! Full-size record character*10 Name_3 (nr__5) ! HD/DM designation integer*4 Teff_3 (nr__5) ! (K) Effective temperature real*4 logg_3 (nr__5) ! ([cm/s2]) Surface gravity real*4 logLum_3 (nr__5) ! ([solLum]) Logaritm of the luminosity in solar unit real*4 v_Fe_H__4 (nr__5) ! ([Sun]) Metallicity real*4 xi_3 (nr__5) ! (km/s) Microturbulent velocity real*4 v_Na_Fe_l_2(nr__5) ! ([Sun]) LTE relative intensity [Na/Fe] real*4 v_Na_Fe_n_2(nr__5) ! ([Sun]) NLTE relative intensity [Na/Fe] real*4 v_Mg_Fe_l (nr__5) ! ([Sun]) LTE relative intensity [Mg/Fe] real*4 v_Mg_Fe_n (nr__5) ! ([Sun]) NLTE relative intensity [Mg/Fe] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table8.dat' ! Na abundances in the 19 program stars integer*4 nr__6 parameter (nr__6=19) ! Number of records character*59 ar__6 ! Full-size record character*10 HD_2 (nr__6) ! HD designation real*4 v_Fe_H__5 (nr__6) ! ([Sun]) Metallicity real*4 v_Na_Fe_1 (nr__6) ! ([Sun]) ? Relative abundance [Na/Fe] from Na I line * at 4751 Angstrom real*4 v_Na_Fe_2 (nr__6) ! ([Sun]) ? Relative abundance [Na/Fe] from Na I line * at 5682 Angstrom real*4 v_Na_Fe_3 (nr__6) ! ([Sun]) ? Relative abundance [Na/Fe] from Na I line * at 5688 Angstrom real*4 v_Na_Fe_4 (nr__6) ! ([Sun]) ? Relative abundance [Na/Fe] from Na I line * at 6154 Angstrom integer*4 Nline (nr__6) ! Number of line for computing the mean real*4 v_Na_Fe_l_3(nr__6) ! ([Sun]) Mean LTE relative abundance [Na/Fe] real*4 e__Na_Fe_l (nr__6) ! ([Sun]) ? rms uncertainty on [Na/Fe]l real*4 v_Na_Fe_n_3(nr__6) ! ([Sun]) Mean NLTE relative abundance [Na/Fe] c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - C Declarations for 'table9.dat' ! Magnesium abundances in the 19 program stars integer*4 nr__7 parameter (nr__7=19) ! Number of records character*50 ar__7 ! Full-size record character*10 HD_3 (nr__7) ! HD designation real*4 v_Fe_H__6 (nr__7) ! ([Sun]) Metallicity real*4 v_Mg_Fe_1 (nr__7) ! ([Sun]) Relative abundance [Mg/Fe] from Mg I line * at 4571 Angstrom real*4 v_Mg_Fe_2 (nr__7) ! ([Sun]) ? Relative abundance [Mg/Fe] from Mg I line * at 4730 Angstrom real*4 v_Mg_Fe_3 (nr__7) ! ([Sun]) ? Relative abundance [Mg/Fe] from Mg I line * at 6318 Angstrom real*4 v_Mg_Fe_4 (nr__7) ! ([Sun]) ? Relative abundance [Mg/Fe] from Mg I line * at 6319 Angstrom integer*4 Nline_1 (nr__7) ! Number of line for computing the mean real*4 v_Mg_Fe__1 (nr__7) ! ([Sun]) Mean LTE relative abundance [Mg/Fe] real*4 e__Mg_Fe_ (nr__7) ! ([Sun]) ? rms uncertainty on [Mg/Fe] C============================================================================= C Loading file 'table2.dat' ! Equivalent widths for O, Na lines in the * 19 program stars and the Sun C Format for file interpretation 1 format( + A10,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,2X,F4.1,1X,F5.1, + 1X,F5.1,1X,F4.1,1X,F4.1,1X,F5.1,1X,F5.1,1X,F4.1) C Effective file loading open(unit=1,status='old',file= +'table2.dat') write(6,*) '....Loading file: table2.dat' do i__=1,20 read(1,'(A77)')ar__ read(ar__,1) + HD(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__), + DEs(i__),EWOI6300(i__),EWOI7771(i__),EWOI7772(i__), + EWOI7774(i__),EWNaI4751(i__),EWNaI5682(i__),EWNaI5688(i__), + EWNaI6154(i__) if(ar__(12:13) .EQ. '') RAh(i__) = iNULL__ if(ar__(15:16) .EQ. '') RAm(i__) = iNULL__ if(ar__(18:21) .EQ. '') RAs(i__) = rNULL__ if(ar__(24:25) .EQ. '') DEd(i__) = iNULL__ if(ar__(27:28) .EQ. '') DEm(i__) = iNULL__ if(ar__(30:31) .EQ. '') DEs(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) + HD(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__), + DEs(i__),EWOI6300(i__),EWOI7771(i__),EWOI7772(i__), + EWOI7774(i__),EWNaI4751(i__),EWNaI5682(i__),EWNaI5688(i__), + EWNaI6154(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 'table3.dat' ! CNO abundances and C12/C13 ratios for the * 19 program stars C Format for file interpretation 2 format( + A10,1X,F5.2,1X,F5.2,1X,F5.2,2X,F5.2,1X,F5.2,2X,F5.2,1X,F5.2, + 1X,F5.2,2X,F5.2,2X,A1,I2,1X,F5.2,1X,F5.2) C Effective file loading open(unit=1,status='old',file= +'table3.dat') write(6,*) '....Loading file: table3.dat' do i__=1,19 read(1,'(A84)')ar__1 read(ar__1,2) + HD_1(i__),v_Fe_H_(i__),v_C_Fe_CH(i__),v_C_Fe_C2(i__), + v_N_Fe_b(i__),v_N_Fe_r(i__),v_N_Fe_(i__),v_O_Fe_1(i__), + v_O_Fe_2(i__),v_O_Fe_(i__),l_C12_C13(i__),C12_C13(i__), + v__C_N__Fe_(i__),v_C_N_(i__) if(ar__1(24:28) .EQ. '') v_C_Fe_C2(i__) = rNULL__ if(ar__1(31:35) .EQ. '') v_N_Fe_b(i__) = rNULL__ if(ar__1(37:41) .EQ. '') v_N_Fe_r(i__) = rNULL__ if(ar__1(44:48) .EQ. '') v_N_Fe_(i__) = rNULL__ if(ar__1(50:54) .EQ. '') v_O_Fe_1(i__) = rNULL__ if(ar__1(56:60) .EQ. '') v_O_Fe_2(i__) = rNULL__ if(ar__1(71:72) .EQ. '') C12_C13(i__) = iNULL__ if(ar__1(80:84) .EQ. '') v_C_N_(i__) = rNULL__ c ..............Just test output........... write(6,2) + HD_1(i__),v_Fe_H_(i__),v_C_Fe_CH(i__),v_C_Fe_C2(i__), + v_N_Fe_b(i__),v_N_Fe_r(i__),v_N_Fe_(i__),v_O_Fe_1(i__), + v_O_Fe_2(i__),v_O_Fe_(i__),l_C12_C13(i__),C12_C13(i__), + v__C_N__Fe_(i__),v_C_N_(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table4.dat' ! Reanalysis of data by Tomkin et al. * (1992AJ....104.1568T) C Format for file interpretation 3 format( + A10,2X,I4,1X,F4.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,A1,F5.2,1X,F4.2, + 1X,F4.2) C Effective file loading open(unit=1,status='old',file= +'table4.dat') write(6,*) '....Loading file: table4.dat' do i__=1,34 read(1,'(A56)')ar__2 read(ar__2,3) + Name(i__),Teff(i__),logg(i__),logLum(i__),v_Fe_H__1(i__), + xi(i__),l__C_Fe_(i__),v_C_Fe_(i__),v_O_Fe_l(i__),v_O_Fe_n(i__) if(ar__2(41:45) .EQ. '') v_C_Fe_(i__) = rNULL__ if(ar__2(47:50) .EQ. '') v_O_Fe_l(i__) = rNULL__ if(ar__2(52:55) .EQ. '') v_O_Fe_n(i__) = rNULL__ c ..............Just test output........... write(6,3) + Name(i__),Teff(i__),logg(i__),logLum(i__),v_Fe_H__1(i__), + xi(i__),l__C_Fe_(i__),v_C_Fe_(i__),v_O_Fe_l(i__),v_O_Fe_n(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table5.dat' ! Reanalysis of data by * Sneden et al. (1991AJ....102.2001S) and * Kraft et al. (1992AJ....104..645K) C Format for file interpretation 4 format( + A10,1X,I4,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2,1X, + F5.2) C Effective file loading open(unit=1,status='old',file= +'table5.dat') write(6,*) '....Loading file: table5.dat' do i__=1,27 read(1,'(A56)')ar__3 read(ar__3,4) + Name_1(i__),Teff_1(i__),logg_1(i__),logLum_1(i__), + v_Fe_H__2(i__),xi_1(i__),v_O_Fe__1(i__),v_Na_Fe_l(i__), + v_Na_Fe_n(i__) if(ar__3(45:49) .EQ. '') v_Na_Fe_l(i__) = rNULL__ if(ar__3(51:55) .EQ. '') v_Na_Fe_n(i__) = rNULL__ c ..............Just test output........... write(6,4) + Name_1(i__),Teff_1(i__),logg_1(i__),logLum_1(i__), + v_Fe_H__2(i__),xi_1(i__),v_O_Fe__1(i__),v_Na_Fe_l(i__), + v_Na_Fe_n(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table6.dat' ! Reanalysis of data by Edvardsson et al. * (1993, Cat. <J/A+A/275/101>) C Format for file interpretation 5 format( + A10,1X,I4,1X,F4.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,A1,F5.2, + 1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2) C Effective file loading open(unit=1,status='old',file= +'table6.dat') write(6,*) '....Loading file: table6.dat' do i__=1,187 read(1,'(A86)')ar__4 read(ar__4,5) + Name_2(i__),Teff_2(i__),logg_2(i__),logLum_2(i__), + v_Fe_H__3(i__),xi_2(i__),v_C_Fe_1(i__),l__C_Fe_2(i__), + v_C_Fe_2(i__),v_O_Fe_1_1(i__),v_O_Fe_2_1(i__),v_O_Fe_3(i__), + v_Na_Fe_l_1(i__),v_Na_Fe_n_1(i__),v_Mg_Fe_(i__) if(ar__4(39:43) .EQ. '') v_C_Fe_1(i__) = rNULL__ if(ar__4(46:50) .EQ. '') v_C_Fe_2(i__) = rNULL__ if(ar__4(52:56) .EQ. '') v_O_Fe_1_1(i__) = rNULL__ if(ar__4(58:62) .EQ. '') v_O_Fe_2_1(i__) = rNULL__ if(ar__4(64:68) .EQ. '') v_O_Fe_3(i__) = rNULL__ if(ar__4(70:74) .EQ. '') v_Na_Fe_l_1(i__) = rNULL__ if(ar__4(76:80) .EQ. '') v_Na_Fe_n_1(i__) = rNULL__ if(ar__4(82:86) .EQ. '') v_Mg_Fe_(i__) = rNULL__ c ..............Just test output........... write(6,5) + Name_2(i__),Teff_2(i__),logg_2(i__),logLum_2(i__), + v_Fe_H__3(i__),xi_2(i__),v_C_Fe_1(i__),l__C_Fe_2(i__), + v_C_Fe_2(i__),v_O_Fe_1_1(i__),v_O_Fe_2_1(i__),v_O_Fe_3(i__), + v_Na_Fe_l_1(i__),v_Na_Fe_n_1(i__),v_Mg_Fe_(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table7.dat' ! Reanalysis of data by Zhao & Magain * (1990A&A...238..242Z) C Format for file interpretation 6 format( + A10,2X,I4,1X,F4.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2,1X, + F4.2,1X,F4.2) C Effective file loading open(unit=1,status='old',file= +'table7.dat') write(6,*) '....Loading file: table7.dat' do i__=1,20 read(1,'(A60)')ar__5 read(ar__5,6) + Name_3(i__),Teff_3(i__),logg_3(i__),logLum_3(i__), + v_Fe_H__4(i__),xi_3(i__),v_Na_Fe_l_2(i__),v_Na_Fe_n_2(i__), + v_Mg_Fe_l(i__),v_Mg_Fe_n(i__) c ..............Just test output........... write(6,6) + Name_3(i__),Teff_3(i__),logg_3(i__),logLum_3(i__), + v_Fe_H__4(i__),xi_3(i__),v_Na_Fe_l_2(i__),v_Na_Fe_n_2(i__), + v_Mg_Fe_l(i__),v_Mg_Fe_n(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table8.dat' ! Na abundances in the 19 program stars C Format for file interpretation 7 format( + A10,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,I1,1X,F5.2,1X, + F4.2,1X,F5.2) C Effective file loading open(unit=1,status='old',file= +'table8.dat') write(6,*) '....Loading file: table8.dat' do i__=1,19 read(1,'(A59)')ar__6 read(ar__6,7) + HD_2(i__),v_Fe_H__5(i__),v_Na_Fe_1(i__),v_Na_Fe_2(i__), + v_Na_Fe_3(i__),v_Na_Fe_4(i__),Nline(i__),v_Na_Fe_l_3(i__), + e__Na_Fe_l(i__),v_Na_Fe_n_3(i__) if(ar__6(18:22) .EQ. '') v_Na_Fe_1(i__) = rNULL__ if(ar__6(24:28) .EQ. '') v_Na_Fe_2(i__) = rNULL__ if(ar__6(30:34) .EQ. '') v_Na_Fe_3(i__) = rNULL__ if(ar__6(36:40) .EQ. '') v_Na_Fe_4(i__) = rNULL__ if(ar__6(50:53) .EQ. '') e__Na_Fe_l(i__) = rNULL__ c ..............Just test output........... write(6,7) + HD_2(i__),v_Fe_H__5(i__),v_Na_Fe_1(i__),v_Na_Fe_2(i__), + v_Na_Fe_3(i__),v_Na_Fe_4(i__),Nline(i__),v_Na_Fe_l_3(i__), + e__Na_Fe_l(i__),v_Na_Fe_n_3(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= C Loading file 'table9.dat' ! Magnesium abundances in the 19 program stars C Format for file interpretation 8 format( + A10,1X,F5.2,1X,F4.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,I1,1X,F4.2,1X, + F4.2) C Effective file loading open(unit=1,status='old',file= +'table9.dat') write(6,*) '....Loading file: table9.dat' do i__=1,19 read(1,'(A50)')ar__7 read(ar__7,8) + HD_3(i__),v_Fe_H__6(i__),v_Mg_Fe_1(i__),v_Mg_Fe_2(i__), + v_Mg_Fe_3(i__),v_Mg_Fe_4(i__),Nline_1(i__),v_Mg_Fe__1(i__), + e__Mg_Fe_(i__) if(ar__7(23:27) .EQ. '') v_Mg_Fe_2(i__) = rNULL__ if(ar__7(29:33) .EQ. '') v_Mg_Fe_3(i__) = rNULL__ if(ar__7(35:38) .EQ. '') v_Mg_Fe_4(i__) = rNULL__ if(ar__7(47:50) .EQ. '') e__Mg_Fe_(i__) = rNULL__ c ..............Just test output........... write(6,8) + HD_3(i__),v_Fe_H__6(i__),v_Mg_Fe_1(i__),v_Mg_Fe_2(i__), + v_Mg_Fe_3(i__),v_Mg_Fe_4(i__),Nline_1(i__),v_Mg_Fe__1(i__), + e__Mg_Fe_(i__) c .......End.of.Just test output........... end do close(1) C============================================================================= stop end