Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/634/1319 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-20
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/634/1319 Synthetic Lick indices of alpha-enhanced stars (Franchini+ 2005)
*================================================================================
*Synthetic Lick indices and detection of {alpha}-enhanced stars.
*III. F, G, and K stars with [Fe/H]>0.00.
* Franchini M., Morossi C., Di Marcantonio P., Castelli F., Malagnini M.L.,
* Chavez M.
* <Astrophys. J., 634, 1319-1335 (2005)>
* =2005ApJ...634.1319F
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! The program stars
integer*4 nr__
parameter (nr__=119) ! Number of records
character*75 ar__ ! Full-size record
character*28 Class (nr__) ! Classification (1)
integer*4 HD (nr__) ! HD number
character*1 f_HD (nr__) ! [+*] Flag on HD (2)
character*10 SpType (nr__) ! MK spectral type
real*4 v_Fe_H_ (nr__) ! ([Sun]) Average log Fe/H number abundance from the
* Taylor catalog
real*4 e__Fe_H_ (nr__) ! ([Sun]) Error in [Fe/H]
character*1 LC (nr__) ! [gd] Luminosity class: giant (g) or dwarf (d)
character*1 W94 (nr__) ! [y-] In the Worthey et al. catalog? (G1)
character*1 C02 (nr__) ! [y-] In the Cananea collection data set? (G2)
character*1 STE (nr__) ! [y-] In the STELIB library data set? (G3)
character*1 ELO (nr__) ! [y-] In the ELODIE library data set? (G4)
character*1 NBP (nr__) ! [y-] In the Nearby Stars Project library data
* set? (G5)
character*1 NSt (nr__) ! [y-] In the NStars library data set? (G6)
character*1 I_US (nr__) ! [y-] In the Indo-US library data set? (G7)
character*1 S4N (nr__) ! [y-] In the Spectroscopic Survey of Stars in
* the Solar Neighborhood database? (G8)
*Note (1): SSA stands for solar scaled abundances, and NSSA for non solar scaled
* abundances (i.e. {alpha}-enhanced stars).
*Note (2): Flag on HD, defined as follows:
* + = NSSA classification from Na D vs Ca4227 diagram only.
* * = SSA classification from Na D vs Mg2 diagram only.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! *Classification of supersolar stars from the literature
integer*4 nr__1
parameter (nr__1=33) ! Number of records
character*174 ar__1 ! Full-size record
integer*4 HD_1 (nr__1) ! The HD number
real*4 v_Fe_H_T (nr__1) ! ([Sun]) ? [Fe/H] value from Taylor catalog
real*4 e__Fe_H_T (nr__1) ! ([Sun]) ? The RMS error in [Fe/H]_T
real*4 dFeT (nr__1) ! ([Sun]) ? Level of supersolar metallicity (1)
real*4 v_Fe_H_1 (nr__1) ! ([Sun]) ? Allende Prieto et al (2004, Cat.
* <J/A+A/420/183>) [Fe/H] value
real*4 e__Fe_H_1 (nr__1) ! ([Sun]) ? The RMS error in [Fe/H]_1
real*4 dFe1 (nr__1) ! ([Sun]) ? Difference if >0 (1)
real*4 v_Fe_H_2 (nr__1) ! ([Sun]) ? Fuhrmann (2004AN....325....3F)
* [Fe/H] value
real*4 e__Fe_H_2 (nr__1) ! ([Sun]) ? The RMS error in [Fe/H]2
real*4 dFe2 (nr__1) ! ([Sun]) ? Difference if >0 (1)
real*4 v_Fe_H_3 (nr__1) ! ([Sun]) ? Bensby et al. (2005, Cat. <J/A+A/433/185>)
* [Fe/H] value
real*4 e__Fe_H_3 (nr__1) ! ([Sun]) ? The RMS error in [Fe/H]3
real*4 dFe3 (nr__1) ! ([Sun]) ? Difference if >0 (1)
real*4 v_Fe_H_4 (nr__1) ! ([Sun]) ? Luck & Heiter (2005AJ....129.1063L)
* [Fe/H] value
real*4 e__Fe_H_4 (nr__1) ! ([Sun]) ? The RMS error in [Fe/H]4
real*4 dFe4 (nr__1) ! ([Sun]) ? Level of supersolar metallicity (1)
real*4 v_Mg_Fe_1 (nr__1) ! ([Sun]) ? Allende Prieto et al (2004, Cat.
* <J/A+A/420/183>) [Mg/Fe] value
real*4 e__Mg_Fe_1 (nr__1) ! ([Sun]) ? The RMS error in [Mg/Fe]1
real*4 dMg1 (nr__1) ! ([Sun]) ? Difference if >0 (1)
real*4 v_Mg_Fe_2 (nr__1) ! ([Sun]) ? Fuhrmann (2004AN....325....3F)
* [Mg/Fe] value
real*4 e__Mg_Fe_2 (nr__1) ! ([Sun]) ? The RMS error in [Mg/Fe]2
real*4 dMg2 (nr__1) ! ([Sun]) ? Difference if >0 (1)
real*4 v_Mg_Fe_3 (nr__1) ! ([Sun]) ? Bensby et al. (2005, Cat.
* <J/A+A/433/185>) [Mg/Fe] value
real*4 e__Mg_Fe_3 (nr__1) ! ([Sun]) ? The RMS error in [Mg/Fe]3
real*4 dMg3 (nr__1) ! ([Sun]) ? Difference if >0 (1)
real*4 v_Mg_Fe_4 (nr__1) ! ([Sun]) ? Luck & Heiter (2005AJ....129.1063L)
* [Mg/Fe] value
real*4 e__Mg_Fe_4 (nr__1) ! ([Sun]) ? The RMS error in [Mg/Fe]4
real*4 dMg4 (nr__1) ! ([Sun]) ? Difference if >0 (1)
character*5 Class_1 (nr__1) ! Star classification (2)
*Note (1): Selected stars have abundance determinations satisfying:
* Diff_Fe_=[Fe/H]-e_[Fe/H]_>0.0dex, with [Fe/H]>0.0dex
* Diff_Mg_=[Mg/Fe]-e_[Mg/Fe]_>0.0dex, with [Mg/Fe]>0.0dex
*Note (2): Possible classification abbreviated as follows:
* SSA = high probability solar-scaled abundance
* SSA: = possible solar-scaled abundance
* NSSA: = possible non-solar-scaled abundance
C=============================================================================
C Loading file 'table2.dat' ! The program stars
C Format for file interpretation
1 format(
+ A28,1X,I6,A1,1X,A10,1X,F4.2,1X,F4.2,1X,A1,1X,A1,1X,A1,1X,A1,
+ 1X,A1,1X,A1,1X,A1,1X,A1,1X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,119
read(1,'(A75)')ar__
read(ar__,1)
+ Class(i__),HD(i__),f_HD(i__),SpType(i__),v_Fe_H_(i__),
+ e__Fe_H_(i__),LC(i__),W94(i__),C02(i__),STE(i__),ELO(i__),
+ NBP(i__),NSt(i__),I_US(i__),S4N(i__)
c ..............Just test output...........
write(6,1)
+ Class(i__),HD(i__),f_HD(i__),SpType(i__),v_Fe_H_(i__),
+ e__Fe_H_(i__),LC(i__),W94(i__),C02(i__),STE(i__),ELO(i__),
+ NBP(i__),NSt(i__),I_US(i__),S4N(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! *Classification of supersolar stars from the literature
C Format for file interpretation
2 format(
+ I6,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,
+ 1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,A5)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,33
read(1,'(A174)')ar__1
read(ar__1,2)
+ HD_1(i__),v_Fe_H_T(i__),e__Fe_H_T(i__),dFeT(i__),
+ v_Fe_H_1(i__),e__Fe_H_1(i__),dFe1(i__),v_Fe_H_2(i__),
+ e__Fe_H_2(i__),dFe2(i__),v_Fe_H_3(i__),e__Fe_H_3(i__),
+ dFe3(i__),v_Fe_H_4(i__),e__Fe_H_4(i__),dFe4(i__),
+ v_Mg_Fe_1(i__),e__Mg_Fe_1(i__),dMg1(i__),v_Mg_Fe_2(i__),
+ e__Mg_Fe_2(i__),dMg2(i__),v_Mg_Fe_3(i__),e__Mg_Fe_3(i__),
+ dMg3(i__),v_Mg_Fe_4(i__),e__Mg_Fe_4(i__),dMg4(i__),
+ Class_1(i__)
if(ar__1(8:12) .EQ. '') v_Fe_H_T(i__) = rNULL__
if(ar__1(14:18) .EQ. '') e__Fe_H_T(i__) = rNULL__
if(ar__1(20:24) .EQ. '') dFeT(i__) = rNULL__
if(ar__1(26:30) .EQ. '') v_Fe_H_1(i__) = rNULL__
if(ar__1(32:36) .EQ. '') e__Fe_H_1(i__) = rNULL__
if(ar__1(38:42) .EQ. '') dFe1(i__) = rNULL__
if(ar__1(44:48) .EQ. '') v_Fe_H_2(i__) = rNULL__
if(ar__1(50:54) .EQ. '') e__Fe_H_2(i__) = rNULL__
if(ar__1(56:60) .EQ. '') dFe2(i__) = rNULL__
if(ar__1(62:66) .EQ. '') v_Fe_H_3(i__) = rNULL__
if(ar__1(68:72) .EQ. '') e__Fe_H_3(i__) = rNULL__
if(ar__1(74:78) .EQ. '') dFe3(i__) = rNULL__
if(ar__1(80:84) .EQ. '') v_Fe_H_4(i__) = rNULL__
if(ar__1(86:90) .EQ. '') e__Fe_H_4(i__) = rNULL__
if(ar__1(92:96) .EQ. '') dFe4(i__) = rNULL__
if(ar__1(98:102) .EQ. '') v_Mg_Fe_1(i__) = rNULL__
if(ar__1(104:108) .EQ. '') e__Mg_Fe_1(i__) = rNULL__
if(ar__1(110:114) .EQ. '') dMg1(i__) = rNULL__
if(ar__1(116:120) .EQ. '') v_Mg_Fe_2(i__) = rNULL__
if(ar__1(122:126) .EQ. '') e__Mg_Fe_2(i__) = rNULL__
if(ar__1(128:132) .EQ. '') dMg2(i__) = rNULL__
if(ar__1(134:138) .EQ. '') v_Mg_Fe_3(i__) = rNULL__
if(ar__1(140:144) .EQ. '') e__Mg_Fe_3(i__) = rNULL__
if(ar__1(146:150) .EQ. '') dMg3(i__) = rNULL__
if(ar__1(152:156) .EQ. '') v_Mg_Fe_4(i__) = rNULL__
if(ar__1(158:162) .EQ. '') e__Mg_Fe_4(i__) = rNULL__
if(ar__1(164:168) .EQ. '') dMg4(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ HD_1(i__),v_Fe_H_T(i__),e__Fe_H_T(i__),dFeT(i__),
+ v_Fe_H_1(i__),e__Fe_H_1(i__),dFe1(i__),v_Fe_H_2(i__),
+ e__Fe_H_2(i__),dFe2(i__),v_Fe_H_3(i__),e__Fe_H_3(i__),
+ dFe3(i__),v_Fe_H_4(i__),e__Fe_H_4(i__),dFe4(i__),
+ v_Mg_Fe_1(i__),e__Mg_Fe_1(i__),dMg1(i__),v_Mg_Fe_2(i__),
+ e__Mg_Fe_2(i__),dMg2(i__),v_Mg_Fe_3(i__),e__Mg_Fe_3(i__),
+ dMg3(i__),v_Mg_Fe_4(i__),e__Mg_Fe_4(i__),dMg4(i__),
+ Class_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end