Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/837/176 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-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/ApJ/837/176 Spectroscopic obs. of 2 red giant stars in omega Cen (Yong+, 2017)
*================================================================================
*A chemical signature from fast-rotating low-metallicity massive stars:
*ROA 276 in {omega} Centauri.
* Yong D., Norris J.E., Da Costa G.S., Stanford L.M., Karakas A.I.,
* Shingles L.J., Hirschi R., Pignatari M.
* <Astrophys. J., 837, 176-176 (2017)>
* =2017ApJ...837..176Y (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Stellar parameters for the program stars
integer*4 nr__
parameter (nr__=2) ! Number of records
character*37 ar__ ! Full-size record
integer*4 ID (nr__) ! Red giant star identifier
integer*4 Teff (nr__) ! (K) [4075/4125] Spectroscopic effective temperature (1)
real*4 logg (nr__) ! ([cm/s2]) [0.2/0.7] Spectroscopic surface gravity (1)
real*4 xi (nr__) ! (km/s) [1.7/2.4] Microturbulent velocity (1)
real*4 v_Fe_H_ (nr__) ! ([Sun]) [-1.8/-1.3] Spectroscopic [Fe/H] abundance
integer*4 Teffp (nr__) ! (K) [4024/4130] Photometric effective temperature
real*4 loggp (nr__) ! ([cm/s2]) [0.3/0.8] Photometric log of surface gravity
*Note (1): The effective temperature, surface gravity, and microturbulent
* velocity ({xi}_t_), were obtained by enforcing excitation and
* ionization balance for Fe lines. The uncertainties in Teff, logg, and
* {xi}_t_ are 50K, 0.2dex, and 0.2km/s, respectively.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Line list, equivalent widths, and abundances
integer*4 nr__1
parameter (nr__1=333) ! Number of records
character*56 ar__1 ! Full-size record
character*5 Ion (nr__1) ! Species identifier
real*8 lambda (nr__1) ! (0.1nm) [4057.8/7947.6]? Wavelength in Angstroms (1)
real*4 LEP (nr__1) ! (eV) [0/5.2]? Lower excitation potential
real*4 log_gf (nr__1) ! ([-]) [-10.3/0.7]? Log oscillator strength
real*4 EW276 (nr__1) ! (10-13m) [20/150]? Equivalent width for ROA 276 (2)
character*1 f_EW276 (nr__1) ! [s] s = spectrum synthesis
real*4 EW46 (nr__1) ! (10-13m) [19.8/150]? Equivalent width for ROA 46 (2)
character*1 f_EW46 (nr__1) ! [s] s = spectrum synthesis
real*4 loge276 (nr__1) ! ([-]) [-1/8.1]? Log abundance for ROA 276
real*4 loge46 (nr__1) ! ([-]) [-1.3/7.6]? Log abundance for ROA 46
integer*4 Ref (nr__1) ! [1/21] Source code (3)
*Note (1): The wavelength range for CH is 4270-4330{AA}.
*Note (2): In units of milli-Angstroms
*Note (3): Code as follows:
* 1 = Masseron et al. (2014, J/A+A/571/A47);
* 2 = Gratton et al. (2003, J/A+A/404/187) and references therein;
* 3 = values as used in Yong et al. (2005A&A...438..875Y) where the
* references include Kurucz & Bell (1995, Atomic line list
* (Cambridge: Smithsonian Astrophysical Observatory)),
* Prochaska et al. (2000AJ....120.2513P),
* Den Hartog et al. (2003ApJS..148..543D),
* Ivans et al. (2001AJ....122.1438I), and
* Ramirez & Cohen (2002AJ....123.3277R);
* 4 = Oxford group including Blackwell et al. (1979MNRAS.186..633B),
* Blackwell et al. (1979MNRAS.186..657B),
* Blackwell et al. (1980MNRAS.191..445B),
* Blackwell et al. (1986MNRAS.220..549B),
* Blackwell et al. (1995A&A...296..217B);
* 5 = Kock & Richter (1968ZA.....69..180K);
* 6 = Hannaford & Lowe (1983OptEn..22..532H);
* 7 = Roederer & Lawler (2012, J/ApJ/750/76);
* 8 = mean of lifetimes from Simsarian et al. (1998PhRvA..57.2448S) and
* Volz & Schmoranzer (1996PhST...65...48V) weighted according to
* uncertainties, via Morton (2000ApJS..130..403M);
* 9 = Wiese F. (2009, CRC Handbook of Chemistry and Physics
* 90th ed. (Boca Raton, FL: CRC Press) 10)
* 10 = Biemont et al. (2011MNRAS.414.3350B);
* 11 = Biemont et al. (1981ApJ...248..867B);
* 12 = Ljung et al. (2006A&A...456.1181L);
* 13 = Whaling & Brault (1988PhyS...38..707W);
* 14 = Davidson et al. (1992A&A...255..457D) using hfs/IS
* from McWilliam (1998AJ....115.1640M);
* 15 = Lawler et al. (2001ApJ...556..452L), using hfs
* from Ivans et al. (2006, J/ApJ/645/613);
* 16 = Lawler et al. (2009, J/ApJS/182/51);
* 17 = Li et al. (2007PhyS...76..577L);
* 18 = Den Hartog et al. (2003ApJS..148..543D), using hfs/IS from
* Roederer et al. (2008ApJ...675..723R) when available;
* 19 = Lawler et al. (2006, J/ApJS/162/227), using hfs/IS from
* Roederer et al. (2008ApJ...675..723R) when available;
* 20 = Lawler et al. (2001ApJ...563.1075L), using hfs/IS
* from Ivans et al. (2006, J/ApJ/645/613);
* 21 = Biemont et al. (2000MNRAS.312..116B), using hfs/IS
* from Roederer et al. (2012ApJS..203...27R).
C=============================================================================
C Loading file 'table1.dat' ! Stellar parameters for the program stars
C Format for file interpretation
1 format(4X,I3,1X,I4,1X,F3.1,1X,F4.2,1X,F5.2,1X,I4,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,2
read(1,'(A37)')ar__
read(ar__,1)
+ ID(i__),Teff(i__),logg(i__),xi(i__),v_Fe_H_(i__),Teffp(i__),
+ loggp(i__)
c ..............Just test output...........
write(6,1)
+ ID(i__),Teff(i__),logg(i__),xi(i__),v_Fe_H_(i__),Teffp(i__),
+ loggp(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Line list, equivalent widths, and abundances
C Format for file interpretation
2 format(
+ A5,1X,F7.2,1X,F4.2,1X,F6.2,1X,F5.1,1X,A1,1X,F5.1,1X,A1,1X,
+ F5.2,1X,F5.2,1X,I2)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,333
read(1,'(A56)')ar__1
read(ar__1,2)
+ Ion(i__),lambda(i__),LEP(i__),log_gf(i__),EW276(i__),
+ f_EW276(i__),EW46(i__),f_EW46(i__),loge276(i__),loge46(i__),
+ Ref(i__)
if(ar__1(7:13) .EQ. '') lambda(i__) = rNULL__
if(ar__1(15:18) .EQ. '') LEP(i__) = rNULL__
if(ar__1(20:25) .EQ. '') log_gf(i__) = rNULL__
if(ar__1(27:31) .EQ. '') EW276(i__) = rNULL__
if(ar__1(35:39) .EQ. '') EW46(i__) = rNULL__
if(ar__1(43:47) .EQ. '') loge276(i__) = rNULL__
if(ar__1(49:53) .EQ. '') loge46(i__) = rNULL__
c ..............Just test output...........
write(6,2)
+ Ion(i__),lambda(i__),LEP(i__),log_gf(i__),EW276(i__),
+ f_EW276(i__),EW46(i__),f_EW46(i__),loge276(i__),loge46(i__),
+ Ref(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end