Conversion of standardized ReadMe file for
file /./ftp/cats/J/AZh/84/997 into FORTRAN code for reading data files line by line.
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/AZh/84/997 Abundances of Sr, Y, Zr, Ce and Ba (Mashonkina+, 2007)
*================================================================================
*Neutron capture elements in halo, thick disk and thin disk stars: strontium,
*yttrium, zirconium, cerium.
* Mashonkina L.I., Vinogradova A.B., Ptitsyn D.A., Khokhlova V.S.,
* Chernetsova T.A.
* <Astron. Zh. 84, 997 (2007)>
* =2007AZh....84..997M
* =2007ARep...51..903M
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'stars.dat' ! Objects with coordinates
integer*4 nr__
parameter (nr__=74) ! Number of records
character*53 ar__ ! Full-size record
C 2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension 2000
real*8 DEdeg ! (deg) Declination 2000
C ---------------------------------- ! (position vector(s) in degrees)
character*10 HD_BD ! HD/BD number
integer*4 RAh ! (h) Right Ascension (2000) (hours)
integer*4 RAm ! (min) Right Ascension (2000) (minutes)
real*8 RAs ! (s) Right Ascension (2000) (seconds)
character*1 DE_ ! Declination (2000) (sign)
integer*4 DEd ! (deg) Declination (2000) (degrees)
integer*4 DEm ! (arcmin) Declination (2000) (minutes)
real*4 DEs ! (arcsec) Declination (2000) (seconds)
character*15 OName ! Other name
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Atomic data and solar abundances for investigated
lines obtained from solar line profile fitting
integer*4 nr__1
parameter (nr__1=15) ! Number of records
character*66 ar__1 ! Full-size record
character*5 Ion ! Species
real*8 lambda ! (0.1nm) Wavelength
real*4 Eexc ! (eV) Excitation energy (1)
integer*4 Mult ! Multiplicity number
real*4 loggf ! ([-]) log of oscillation strength
integer*4 Ref ! Reference (2)
real*4 logC6 ! C_6_ abundance
character*1 n_logC6 ! [1-3] Origin of logC6 (3)
real*4 log_eps ! ([-]) Solar abundance (H=12)
character*13 Rem ! Remarks
*Note (1): According to Moore, 1972, A multiplet table of astrophysical
* interest, NSRD-NBS 40 (Washington, D.C.).
*Note (2): References as follows:
* 13 = Kurucz, 1994, CD-ROM Nos 18, 19
* 23 = Hannaford et al., 1982ApJ...261..736H
* 26 = Brage et al., 1998ApJ...496.1051B
* 27 = Ljung et al., 2006A&A...456.1181L
* 28 = Palmeri et al., 2000, Phys. Scr. 61, 323
* 29 = Reader et al., Wavelengths and Transaction Probabilities for
* atoms and atomic ions, PartII, NSRD-NBS 68 (Washington, D.C., 1980)
*Note (3): Note as follows:
* 1 = based on profile analysis for the solar spectrum
* 2 = data of Kurucz, CD-ROM Nos 18, 19
* 3 = data of Barklem et O'Mara, 1998MNRAS.300..863B
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Stellar parameters and element abundance ratios
of the stars with [Fe/H]>-0.9
integer*4 nr__2
parameter (nr__2=54) ! Number of records
character*70 ar__2 ! Full-size record
character*10 HD_BD_1 ! HD number
integer*4 Teff ! (K) Effective temperature
real*4 logg ! Surface gravity
real*4 v_Fe_H_ ! Iron abundance
real*4 VT ! (km/s) Microturbulence velocity
integer*4 Code ! [0/3] Stellar population type (1)
real*4 v_Sr_Fe_ ! ? Strontium to Fe abundance
real*4 v_Y_Fe_ ! ? Yttrium to Fe abundance
real*4 v_Zr_Fe_ ! ? Zirconium to Fe abundance
real*4 v_Ba_Fe_ ! Barium to Fe abundance
real*4 v_Ce_Fe_ ! ? Cerium to Fe abundance
*Note (1): population is coded as follows:
* 0 = thin disk
* 1 = thick disk
* 2 = halo
* 3 = transition phase between thin and thick disks
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Stellar parameters and element abundance ratios
of the stars with [Fe/H]<-0.9
integer*4 nr__3
parameter (nr__3=20) ! Number of records
character*70 ar__3 ! Full-size record
character*10 HD_BD_2 ! HD number
integer*4 Teff_1 ! (K) Effective temperature
real*4 logg_1 ! Surface gravity
real*4 v_Fe_H__1 ! Iron abundance
real*4 VT_1 ! (km/s) Microturbulence velocity
integer*4 Code_1 ! [0/3] Stellar population type (1)
real*4 v_Sr_Fe__1 ! ? Strontium to Fe abundance
real*4 v_Y_Fe__1 ! ? Yttrium to Fe abundance
real*4 v_Zr_Fe__1 ! ? Zirconium to Fe abundance
real*4 v_Ba_Fe__1 ! Barium to Fe abundance
real*4 v_Ce_Fe__1 ! ? Cerium to Fe abundance
*Note (1): population is coded as follows:
* 0 = thin disk
* 1 = thick disk
* 2 = halo
* 3 = transition phase between thin and thick disks
C=============================================================================
C Loading file 'stars.dat' ! Objects with coordinates
C Format for file interpretation
1 format(A10,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F6.3,1X,A15)
C Effective file loading
open(unit=1,status='old',file=
+'stars.dat')
write(6,*) '....Loading file: stars.dat'
do i__=1,74
read(1,'(A53)')ar__
read(ar__,1)HD_BD,RAh,RAm,RAs,DE_,DEd,DEm,DEs,OName
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)HD_BD,RAh,RAm,RAs,DE_,DEd,DEm,DEs,OName
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table1.dat' ! Atomic data and solar abundances for investigated
* lines obtained from solar line profile fitting
C Format for file interpretation
2 format(
+ A5,2X,F7.2,2X,F5.3,2X,I2,1X,F6.3,2X,I2,2X,F6.2,1X,A1,1X,F4.2,
+ 2X,A13)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,15
read(1,'(A66)')ar__1
read(ar__1,2)
+ Ion,lambda,Eexc,Mult,loggf,Ref,logC6,n_logC6,log_eps,Rem
c ..............Just test output...........
write(6,2)
+ Ion,lambda,Eexc,Mult,loggf,Ref,logC6,n_logC6,log_eps,Rem
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Stellar parameters and element abundance ratios
* of the stars with [Fe/H]>-0.9
C Format for file interpretation
3 format(
+ A10,1X,I4,2X,F4.2,2X,F5.2,2X,F3.1,2X,I1,2X,F5.2,2X,F5.2,1X,
+ F5.2,2X,F5.2,2X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,54
read(1,'(A70)')ar__2
read(ar__2,3)
+ HD_BD_1,Teff,logg,v_Fe_H_,VT,Code,v_Sr_Fe_,v_Y_Fe_,v_Zr_Fe_,
+ v_Ba_Fe_,v_Ce_Fe_
if(ar__2(39:43) .EQ. '') v_Sr_Fe_ = rNULL__
if(ar__2(46:50) .EQ. '') v_Y_Fe_ = rNULL__
if(ar__2(52:56) .EQ. '') v_Zr_Fe_ = rNULL__
if(ar__2(66:70) .EQ. '') v_Ce_Fe_ = rNULL__
c ..............Just test output...........
write(6,3)
+ HD_BD_1,Teff,logg,v_Fe_H_,VT,Code,v_Sr_Fe_,v_Y_Fe_,v_Zr_Fe_,
+ v_Ba_Fe_,v_Ce_Fe_
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Stellar parameters and element abundance ratios
* of the stars with [Fe/H]<-0.9
C Format for file interpretation
4 format(
+ A10,1X,I4,2X,F4.2,2X,F5.2,2X,F3.1,2X,I1,2X,F5.2,2X,F5.2,1X,
+ F5.2,2X,F5.2,2X,F5.2)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,20
read(1,'(A70)')ar__3
read(ar__3,4)
+ HD_BD_2,Teff_1,logg_1,v_Fe_H__1,VT_1,Code_1,v_Sr_Fe__1,
+ v_Y_Fe__1,v_Zr_Fe__1,v_Ba_Fe__1,v_Ce_Fe__1
if(ar__3(39:43) .EQ. '') v_Sr_Fe__1 = rNULL__
if(ar__3(46:50) .EQ. '') v_Y_Fe__1 = rNULL__
if(ar__3(52:56) .EQ. '') v_Zr_Fe__1 = rNULL__
if(ar__3(66:70) .EQ. '') v_Ce_Fe__1 = rNULL__
c ..............Just test output...........
write(6,4)
+ HD_BD_2,Teff_1,logg_1,v_Fe_H__1,VT_1,Code_1,v_Sr_Fe__1,
+ v_Y_Fe__1,v_Zr_Fe__1,v_Ba_Fe__1,v_Ce_Fe__1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end