Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/122/2569 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/122/2569 VI photometry of NGC 288, 362 and 1851 (Bellazzini+, 2001)
*================================================================================
*Age as the second parameter in NGC 288/NGC 362?
*I. Turnoff ages: a purely differential comparison.
* Bellazzini M., Pecci F.F., Ferraro F.R., Galleti S., Catelan M.,
* Landsman W.B.
* <Astron. J. 122, 2569 (2001)>
* =2001AJ....122.2569B
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! Photometry of NGC 288
integer*4 nr__
parameter (nr__=10990) ! Number of records
character*65 ar__ ! Full-size record
integer*4 BPF (nr__) ! Object identification (1)
real*4 Vmag (nr__) ! (mag) The V band magnitude
real*4 e_Vmag (nr__) ! (mag) Error in Vmag
real*4 Imag (nr__) ! (mag) The I band magnitude
real*4 e_Imag (nr__) ! (mag) Error in Imag
real*8 Xpix (nr__) ! (pix) The X pixel position (2)
real*8 Ypix (nr__) ! (pix) The Y pixel position (2)
character*8 Name (nr__) ! Other object identification (3)
*Note (1): In Simbad, the designations are:
* Cl* NGC 288 BPF NNNNN in table1.dat
* Cl* NGC 1851 BPF NNNN in table2.dat
* Cl* NGC 362 BPF NNNN in table3.dat
*Note (2): 1 pix = 0.26"
*Note (3): Other object identification:
* V# = Cl* NGC AAAA SAW VNN in Simbad e.g.
* Cl* NGC 288 Saw VN, RR Lyrae variables found by Kaluzny
* (1996A&AS..120...83K) in table1.dat,
* Cl* NGC 1851 SAW VNN, RR Lyrae variables in common with Walker
* (1998AJ....116..220W) in table2.dat
* Cl* NGC 362 SAW VNNN, RR Lyrae variables identified in the
* Sawyer-Hogg (1973, updated by C. Clement, 1997, Cat. <V/97>),
* in table3.dat
* Guo 4110 = A non member star identified in the proper motions database
* by Guo (1995, Ph.D. thesis, Yale Univ.);
* EHB1 = The extreme HB star identified by Bellazzini & Messineo (1999,
* in The Chemical Evolution of the Milky Way: Stars versus
* Clusters, ed. F. Matteucci & F. Giovannelli (Dordrecht:
* Kluwer), 213).
* UIT-# = UV sources identified by the UIT satellite (see Cat. <VI/104>)
* PNM = probable non member (only for stars near the HB) according to
* Tucholke (1992, Cat. <J/A+AS/93/311>).
* MJ #### = Cl* NGC 362 MJ NNNNN, BHB star that is a confirmed member of the
* cluster according to Moehler et al. (2000A&A...361..937M).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Photometry of NGC 1851
integer*4 nr__1
parameter (nr__1=9118) ! Number of records
character*65 ar__1 ! Full-size record
integer*4 BPF_1 (nr__1) ! Object identification (1)
real*4 Vmag_1 (nr__1) ! (mag) The V band magnitude
real*4 e_Vmag_1 (nr__1) ! (mag) Error in Vmag
real*4 Imag_1 (nr__1) ! (mag) The I band magnitude
real*4 e_Imag_1 (nr__1) ! (mag) Error in Imag
real*8 Xpix_1 (nr__1) ! (pix) The X pixel position (2)
real*8 Ypix_1 (nr__1) ! (pix) The Y pixel position (2)
character*8 Name_1 (nr__1) ! Other object identification (3)
*Note (1): In Simbad, the designations are:
* Cl* NGC 288 BPF NNNNN in table1.dat
* Cl* NGC 1851 BPF NNNN in table2.dat
* Cl* NGC 362 BPF NNNN in table3.dat
*Note (2): 1 pix = 0.26"
*Note (3): Other object identification:
* V# = Cl* NGC AAAA SAW VNN in Simbad e.g.
* Cl* NGC 288 Saw VN, RR Lyrae variables found by Kaluzny
* (1996A&AS..120...83K) in table1.dat,
* Cl* NGC 1851 SAW VNN, RR Lyrae variables in common with Walker
* (1998AJ....116..220W) in table2.dat
* Cl* NGC 362 SAW VNNN, RR Lyrae variables identified in the
* Sawyer-Hogg (1973, updated by C. Clement, 1997, Cat. <V/97>),
* in table3.dat
* Guo 4110 = A non member star identified in the proper motions database
* by Guo (1995, Ph.D. thesis, Yale Univ.);
* EHB1 = The extreme HB star identified by Bellazzini & Messineo (1999,
* in The Chemical Evolution of the Milky Way: Stars versus
* Clusters, ed. F. Matteucci & F. Giovannelli (Dordrecht:
* Kluwer), 213).
* UIT-# = UV sources identified by the UIT satellite (see Cat. <VI/104>)
* PNM = probable non member (only for stars near the HB) according to
* Tucholke (1992, Cat. <J/A+AS/93/311>).
* MJ #### = Cl* NGC 362 MJ NNNNN, BHB star that is a confirmed member of the
* cluster according to Moehler et al. (2000A&A...361..937M).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Photometry of NGC 362
integer*4 nr__2
parameter (nr__2=7492) ! Number of records
character*65 ar__2 ! Full-size record
integer*4 BPF_2 (nr__2) ! Object identification (1)
real*4 Vmag_2 (nr__2) ! (mag) The V band magnitude
real*4 e_Vmag_2 (nr__2) ! (mag) Error in Vmag
real*4 Imag_2 (nr__2) ! (mag) The I band magnitude
real*4 e_Imag_2 (nr__2) ! (mag) Error in Imag
real*8 Xpix_2 (nr__2) ! (pix) The X pixel position (2)
real*8 Ypix_2 (nr__2) ! (pix) The Y pixel position (2)
character*8 Name_2 (nr__2) ! Other object identification (3)
*Note (1): In Simbad, the designations are:
* Cl* NGC 288 BPF NNNNN in table1.dat
* Cl* NGC 1851 BPF NNNN in table2.dat
* Cl* NGC 362 BPF NNNN in table3.dat
*Note (2): 1 pix = 0.26"
*Note (3): Other object identification:
* V# = Cl* NGC AAAA SAW VNN in Simbad e.g.
* Cl* NGC 288 Saw VN, RR Lyrae variables found by Kaluzny
* (1996A&AS..120...83K) in table1.dat,
* Cl* NGC 1851 SAW VNN, RR Lyrae variables in common with Walker
* (1998AJ....116..220W) in table2.dat
* Cl* NGC 362 SAW VNNN, RR Lyrae variables identified in the
* Sawyer-Hogg (1973, updated by C. Clement, 1997, Cat. <V/97>),
* in table3.dat
* Guo 4110 = A non member star identified in the proper motions database
* by Guo (1995, Ph.D. thesis, Yale Univ.);
* EHB1 = The extreme HB star identified by Bellazzini & Messineo (1999,
* in The Chemical Evolution of the Milky Way: Stars versus
* Clusters, ed. F. Matteucci & F. Giovannelli (Dordrecht:
* Kluwer), 213).
* UIT-# = UV sources identified by the UIT satellite (see Cat. <VI/104>)
* PNM = probable non member (only for stars near the HB) according to
* Tucholke (1992, Cat. <J/A+AS/93/311>).
* MJ #### = Cl* NGC 362 MJ NNNNN, BHB star that is a confirmed member of the
* cluster according to Moehler et al. (2000A&A...361..937M).
C=============================================================================
C Loading file 'table1.dat' ! Photometry of NGC 288
C Format for file interpretation
1 format(I5,2X,F6.3,2X,F5.3,2X,F6.3,2X,F5.3,3X,F7.2,2X,F8.2,2X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,10990
read(1,'(A65)')ar__
read(ar__,1)
+ BPF(i__),Vmag(i__),e_Vmag(i__),Imag(i__),e_Imag(i__),
+ Xpix(i__),Ypix(i__),Name(i__)
c ..............Just test output...........
write(6,1)
+ BPF(i__),Vmag(i__),e_Vmag(i__),Imag(i__),e_Imag(i__),
+ Xpix(i__),Ypix(i__),Name(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Photometry of NGC 1851
C Format for file interpretation
2 format(I5,2X,F6.3,2X,F5.3,2X,F6.3,2X,F5.3,3X,F7.2,2X,F8.2,2X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,9118
read(1,'(A65)')ar__1
read(ar__1,2)
+ BPF_1(i__),Vmag_1(i__),e_Vmag_1(i__),Imag_1(i__),
+ e_Imag_1(i__),Xpix_1(i__),Ypix_1(i__),Name_1(i__)
c ..............Just test output...........
write(6,2)
+ BPF_1(i__),Vmag_1(i__),e_Vmag_1(i__),Imag_1(i__),
+ e_Imag_1(i__),Xpix_1(i__),Ypix_1(i__),Name_1(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table3.dat' ! Photometry of NGC 362
C Format for file interpretation
3 format(I5,2X,F6.3,2X,F5.3,2X,F6.3,2X,F5.3,3X,F7.2,2X,F8.2,2X,A8)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,7492
read(1,'(A65)')ar__2
read(ar__2,3)
+ BPF_2(i__),Vmag_2(i__),e_Vmag_2(i__),Imag_2(i__),
+ e_Imag_2(i__),Xpix_2(i__),Ypix_2(i__),Name_2(i__)
c ..............Just test output...........
write(6,3)
+ BPF_2(i__),Vmag_2(i__),e_Vmag_2(i__),Imag_2(i__),
+ e_Imag_2(i__),Xpix_2(i__),Ypix_2(i__),Name_2(i__)
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end