Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/103/1987 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/AJ/103/1987 Stars of very low metal abundance (Beers+ 1992)
*================================================================================
*A search for stars of very low metal abundance. II.
* Beers T.C., Preston G.W., Shectman S.A.
* <Astron. J. 103, 1987 (1992)>
* =1992AJ....103.1987B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table5.dat' ! Observational data, derived distances, and abundances
integer*4 nr__
parameter (nr__=1044) ! Number of records
character*136 ar__ ! Full-size record
C 1950 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg (nr__) ! (deg) Right Ascension 1950
real*8 DEdeg (nr__) ! (deg) Declination 1950
C ---------------------------------- ! (position vector(s) in degrees)
character*9 BPS_CS (nr__) ! Star designation
integer*4 RAh (nr__) ! (h) Right Ascension 1950 (hours)
integer*4 RAm (nr__) ! (min) Right Ascension 1950 (minutes)
real*4 RAs (nr__) ! (s) Right Ascension 1950 (seconds)
character*1 DE_ (nr__) ! Declination 1950 (sign)
integer*4 DEd (nr__) ! (deg) Declination 1950 (degrees)
integer*4 DEm (nr__) ! (arcmin) Declination 1950 (minutes)
integer*4 DEs (nr__) ! (arcsec) Declination 1950 (seconds)
real*4 GLON (nr__) ! (deg) Galactic longitude
real*4 GLAT (nr__) ! (deg) Galactic latitude
real*4 Vmag (nr__) ! (mag) ? Johnson V magnitude
real*4 B_V (nr__) ! (mag) ? Johnson B-V color
real*4 U_B (nr__) ! (mag) ? Johnson U-B color
real*4 E_B_V (nr__) ! (mag) B-V excess
real*4 BV (nr__) ! (mag) ? BV color estimate, obtained from calibration
* of Balmer Index HP
integer*4 RV (nr__) ! (km/s) Radial velocity
character*3 Det (nr__) ! Detector Identification:
* R = Reticon; F = 2D-Frutti; R/F = both
real*4 KP (nr__) ! (0.1nm) CaII K equivalent width index KP (Angstroms)
real*4 HP (nr__) ! (0.1nm) ? Balmer line equivalent width index HP (1)
real*4 GP (nr__) ! (0.1nm) ? G-band equivalent width index GP (Angstroms)
character*3 Class (nr__) ! Classification of stellar type
real*4 Mv (nr__) ! (mag) ? Absolute magnitude estimate
real*4 Dist (nr__) ! (kpc) ? Distance estimate (kpc)
real*4 Wk (nr__) ! (0.1nm) ? Interstellar CaII K estimate
* (as in Beers 1990AJ.....99..323B)
real*4 v_Fe_H_k (nr__) ! (Sun) ? estimate from Norris models
real*4 v_Fe_H_c (nr__) ! (Sun) ? adopted estimate
character*1 D (nr__) ! [D] indicates duplicity, see the list in
* the "Duplicated stars" section below.
*Note (1): HP is an average of H lines:
* HP = -0.276 + 0.5H{delta} + 0.588H{gamma}
C=============================================================================
C Loading file 'table5.dat' ! Observational data, derived distances, and abundances
C Format for file interpretation
1 format(
+ 3X,A9,1X,I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,I2,1X,F5.1,1X,
+ F5.1,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F4.2,1X,I4,1X,A3,1X,
+ F5.2,1X,F5.2,1X,F5.2,1X,A3,1X,F5.2,1X,F4.1,1X,F5.2,1X,F5.2,1X,
+ F5.2,2X,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table5.dat')
write(6,*) '....Loading file: table5.dat'
do i__=1,1044
read(1,'(A136)')ar__
read(ar__,1)
+ BPS_CS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),GLON(i__),GLAT(i__),Vmag(i__),B_V(i__),
+ U_B(i__),E_B_V(i__),BV(i__),RV(i__),Det(i__),KP(i__),HP(i__),
+ GP(i__),Class(i__),Mv(i__),Dist(i__),Wk(i__),v_Fe_H_k(i__),
+ v_Fe_H_c(i__),D(i__)
if(ar__(47:51) .EQ. '') Vmag(i__) = rNULL__
if(ar__(53:57) .EQ. '') B_V(i__) = rNULL__
if(ar__(59:63) .EQ. '') U_B(i__) = rNULL__
if(ar__(70:73) .EQ. '') BV(i__) = rNULL__
if(ar__(90:94) .EQ. '') HP(i__) = rNULL__
if(ar__(96:100) .EQ. '') GP(i__) = rNULL__
if(ar__(106:110) .EQ. '') Mv(i__) = rNULL__
if(ar__(112:115) .EQ. '') Dist(i__) = rNULL__
if(ar__(117:121) .EQ. '') Wk(i__) = rNULL__
if(ar__(123:127) .EQ. '') v_Fe_H_k(i__) = rNULL__
if(ar__(129:133) .EQ. '') v_Fe_H_c(i__) = rNULL__
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)
+ BPS_CS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
+ DEm(i__),DEs(i__),GLON(i__),GLAT(i__),Vmag(i__),B_V(i__),
+ U_B(i__),E_B_V(i__),BV(i__),RV(i__),Det(i__),KP(i__),HP(i__),
+ GP(i__),Class(i__),Mv(i__),Dist(i__),Wk(i__),v_Fe_H_k(i__),
+ v_Fe_H_c(i__),D(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end