Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_AS/124/353 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-Jun-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. J/A+AS/124/353 CCD UBV photometry of close visual doubles (Nakos+ 1997)
*================================================================================
*UBV absolute CCD photometry and differential astrometry of
*close visual double stars, with G-type primaries.
* Nakos T., Sinachopoulos D., van Dessel E.
* <Astron. Astrophys. Suppl. Ser. 124, 353 (1997)>
* =1997A&AS..124..353N (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1' ! Astrometric results
integer*4 nr__
parameter (nr__=39) ! Number of records
character*58 ar__ ! Full-size record
C J2000 position composed of: RAh RAm DE- DEd DEm
real*8 RAdeg (nr__) ! (deg) Right Ascension J2000
real*8 DEdeg (nr__) ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 No (nr__) ! Visual binary number
integer*4 RAh (nr__) ! (h) Right ascension (J2000)
real*4 RAm (nr__) ! (min) Right ascension (J2000)
character*1 DE_ (nr__) ! Declination sign
integer*4 DEd (nr__) ! (deg) Declination (J2000)
integer*4 DEm (nr__) ! (arcmin) Declination (J2000)
character*9 DM (nr__) ! Durchmusterung designation of the primary
real*4 rho (nr__) ! (arcsec) Angular separation
real*4 e_rho (nr__) ! (arcsec) rms uncertainty on rho (1)
real*8 Theta (nr__) ! (deg) Position angle
real*4 e_Theta (nr__) ! (deg) rms uncertainty on Theta
real*4 Obs (nr__) ! (yr) Epoch of observation
*Note (1): The very small values of e_rho are due to the assumption of
* {sigma}_r_({rho})=0. We took {sigma}_r_({rho})=0 for the error
* of the angular separation rho due to the atmospheric refraction.
* Realistic values of e_rho are probably one order of magnitude higher
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2' ! Photometric results
integer*4 nr__1
parameter (nr__1=80) ! Number of records
character*45 ar__1 ! Full-size record
integer*4 No_1 (nr__1) ! Visual binary number
character*9 DM_1 (nr__1) ! DM number
character*1 m_DM (nr__1) ! Multiplicity index on DM
real*4 Vmag (nr__1) ! (mag) V magnitude
real*4 e_Vmag (nr__1) ! (mag) rms uncertainty on Vmag
real*4 B_V (nr__1) ! (mag) B-V colour index
real*4 e_B_V (nr__1) ! (mag) rms uncertainty on B-V
real*4 U_B (nr__1) ! (mag) U-B colour index
real*4 e_U_B (nr__1) ! (mag) rms uncertainty on U-B
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3' ! Photometric differences and angular separation
of the components
integer*4 nr__2
parameter (nr__2=40) ! Number of records
character*38 ar__2 ! Full-size record
integer*4 No_2 (nr__2) ! Visual binary number
character*9 DM_2 (nr__2) ! DM or ADS number
real*4 rho_1 (nr__2) ! (arcsec) ? Angular separation
real*4 DVmag (nr__2) ! (mag) Difference in V magnitude
real*4 D_B_V (nr__2) ! (mag) Difference in B-V colour index
real*4 D_U_B (nr__2) ! (mag) Difference in U-B colour index
C=============================================================================
C Loading file 'table1' ! Astrometric results
C Format for file interpretation
1 format(
+ I3,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,A9,1X,F5.3,1X,F4.3,1X,F7.3,
+ 1X,F3.2,1X,F6.1)
C Effective file loading
open(unit=1,status='old',file=
+'table1')
write(6,*) '....Loading file: table1'
do i__=1,39
read(1,'(A58)')ar__
read(ar__,1)
+ No(i__),RAh(i__),RAm(i__),DE_(i__),DEd(i__),DEm(i__),DM(i__),
+ rho(i__),e_rho(i__),Theta(i__),e_Theta(i__),Obs(i__)
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(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c ..............Just test output...........
write(6,1)
+ No(i__),RAh(i__),RAm(i__),DE_(i__),DEd(i__),DEm(i__),DM(i__),
+ rho(i__),e_rho(i__),Theta(i__),e_Theta(i__),Obs(i__)
write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2' ! Photometric results
C Format for file interpretation
2 format(
+ I2,1X,A9,A1,1X,F6.3,1X,F3.2,1X,F5.3,1X,F3.2,1X,F6.3,1X,F3.2)
C Effective file loading
open(unit=1,status='old',file=
+'table2')
write(6,*) '....Loading file: table2'
do i__=1,80
read(1,'(A45)')ar__1
read(ar__1,2)
+ No_1(i__),DM_1(i__),m_DM(i__),Vmag(i__),e_Vmag(i__),B_V(i__),
+ e_B_V(i__),U_B(i__),e_U_B(i__)
c ..............Just test output...........
write(6,2)
+ No_1(i__),DM_1(i__),m_DM(i__),Vmag(i__),e_Vmag(i__),B_V(i__),
+ e_B_V(i__),U_B(i__),e_U_B(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3' ! Photometric differences and angular separation
* of the components
C Format for file interpretation
3 format(I2,1X,A9,1X,F5.3,1X,F5.3,1X,F6.3,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'table3')
write(6,*) '....Loading file: table3'
do i__=1,40
read(1,'(A38)')ar__2
read(ar__2,3)
+ No_2(i__),DM_2(i__),rho_1(i__),DVmag(i__),D_B_V(i__),
+ D_U_B(i__)
if(ar__2(14:18) .EQ. '') rho_1(i__) = rNULL__
c ..............Just test output...........
write(6,3)
+ No_2(i__),DM_2(i__),rho_1(i__),DVmag(i__),D_B_V(i__),
+ D_U_B(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end