Conversion of standardized ReadMe file for
file /./ftp/cats/II/44 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-Jul-13
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. II/44 K-Line photometry of stars in Population I clusters (Hesser+ 1971)
*================================================================================
*K-line photometry of stars in Population I clusters,
* Hesser J.E., Henry R.C.
* <Astrophys. J. Suppl., 23, 453 (1971)>
* =1971ApJS...23..453H
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'data.dat' ! Results (tables 1-6)
integer*4 nr__
parameter (nr__=168) ! Number of records
character*127 ar__ ! Full-size record
character*8 Cl (nr__) ! Cluster name (1)
integer*4 Star (nr__) ! Star number in cluster (1)
real*4 Vmag (nr__) ! (mag) V-band magnitude
real*4 B_V (nr__) ! (mag) (B-V) color index
real*4 m1 (nr__) ! (mag) m_1_ Stroemgren index
real*4 c1 (nr__) ! (mag) ? c_1_ Stroemgren index
real*4 k (nr__) ! (mag) Ca K-line index (3934{AA})
real*4 e_k (nr__) ! (mag) ? RMS error on k
real*4 dk (nr__) ! (mag) Deviation of k-index from normal value
character*1 Sg (nr__) ! [EIL] Stroemgren's group (Early, Intermediate
* or Late)
real*4 b_y (nr__) ! (mag) ? (b-y) color index, reddening corrected
real*4 E_b_y (nr__) ! (mag) ? Reddening in (b-y)
real*4 beta (nr__) ! (mag) ? H{beta} Stroemgren index
real*4 v_m1_ (nr__) ! (mag) ? reddening-independent metallicity index [m_1_]
real*4 d_m1_ (nr__) ! (mag) ? Deviation of [m_1_] from normal
real*4 v_c1_ (nr__) ! (mag) ? reddening-independent luminosity index [c_1_]
real*4 dV (nr__) ! (mag) ? Deviation of V from main sequence
real*4 u_b (nr__) ! (mag) ? luminosity/temperature color index
real*4 a (nr__) ! (mag) ? Temperature parameter (2)
*Note (1): Star numbers refer to:
* * NGC 6475: Koelbloed (1959BAN....14..265K)
* * Orion: number from Brun (1935POLyo...1...12B)
* * Pleiades: number from Hertzsprung (1947AnLei..19a...1H),
* <Cl Melotte 22 NNN> in Simbad
* * IC 2391: HD number
* * IC 2602: HD(E) number, except star #57 is from Braes (1962BAN....16..297B)
* * Hyades: HD number
*Note (2): temperature index:
* * for stars of the early-group (E), the value is {delta}[m_1_],
* calculated by the alternate method
* * for stars of the intermediate group (early A stars), it is defined as:
* a = (b-y) + 0.189[(u-b) - 1.36mag]
C=============================================================================
C Loading file 'data.dat' ! Results (tables 1-6)
C Format for file interpretation
1 format(
+ A8,6X,I6,1X,F5.2,1X,F5.2,1X,F6.3,1X,F6.3,1X,F6.3,1X,F5.3,1X,
+ F6.3,2X,A1,1X,F6.3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F6.3,1X,F5.3,2X,
+ F4.2,1X,F5.3,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'data.dat')
write(6,*) '....Loading file: data.dat'
do i__=1,168
read(1,'(A127)')ar__
read(ar__,1)
+ Cl(i__),Star(i__),Vmag(i__),B_V(i__),m1(i__),c1(i__),k(i__),
+ e_k(i__),dk(i__),Sg(i__),b_y(i__),E_b_y(i__),beta(i__),
+ v_m1_(i__),d_m1_(i__),v_c1_(i__),dV(i__),u_b(i__),a(i__)
if(ar__(41:46) .EQ. '') c1(i__) = rNULL__
if(ar__(55:59) .EQ. '') e_k(i__) = rNULL__
if(ar__(71:76) .EQ. '') b_y(i__) = rNULL__
if(ar__(78:83) .EQ. '') E_b_y(i__) = rNULL__
if(ar__(85:89) .EQ. '') beta(i__) = rNULL__
if(ar__(91:95) .EQ. '') v_m1_(i__) = rNULL__
if(ar__(97:102) .EQ. '') d_m1_(i__) = rNULL__
if(ar__(104:108) .EQ. '') v_c1_(i__) = rNULL__
if(ar__(111:114) .EQ. '') dV(i__) = rNULL__
if(ar__(116:120) .EQ. '') u_b(i__) = rNULL__
if(ar__(122:127) .EQ. '') a(i__) = rNULL__
c ..............Just test output...........
write(6,1)
+ Cl(i__),Star(i__),Vmag(i__),B_V(i__),m1(i__),c1(i__),k(i__),
+ e_k(i__),dk(i__),Sg(i__),b_y(i__),E_b_y(i__),beta(i__),
+ v_m1_(i__),d_m1_(i__),v_c1_(i__),dV(i__),u_b(i__),a(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end