Conversion of standardized ReadMe file for
file /./ftp/cats/J/AJ/116/723 into FORTRAN code for reading data files line by line.
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/116/723 LMC star clusters ages and metallicity (Bica+ 1998)
*================================================================================
*Ages and metallicities of star clusters and surrounding fields in the outer disk
*of the Large Magellanic Cloud.
* Bica E., Geisler D., Dottori H., Claria J.J., Piatti A.E.,
* Santos J.F.C.Jr
* <Astron. J. 116, 723 (1998)>
* =1998AJ....116..723B (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tab134.dat' ! Sample of outlying clusters and surrounding
fields, ages, reddenings and metallicities
integer*4 nr__
parameter (nr__=14) ! Number of records
character*108 ar__ ! Full-size record
C B1950.0 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension B1950.0
real*8 DEdeg ! (deg) Declination B1950.0
C ---------------------------------- ! (position vector(s) in degrees)
character*12 Cluster ! Star cluster designation
character*14 OtherName ! Other name of the star cluster
integer*4 RAh ! (h) Right ascension (B1950.0)
integer*4 RAm ! (min) Right ascension (B1950.0)
integer*4 RAs ! (s) Right ascension (B1950.0)
character*1 DE_ ! Declination sign
integer*4 DEd ! (deg) Declination (B1950.0)
integer*4 DEm ! (arcmin) Declination (B1950.0)
integer*4 DEs ! (arcsec) Declination (B1950.0)
real*4 GLON ! (deg) Galactic longitude
real*4 GLAT ! (deg) Galactic latitude
real*4 Rad ! (deg) Cluster radius
real*4 R ! (deg) Deprojected angular distance
character*1 Note ! [abc] Note (1)
real*4 AgeCluster ! (Gyr) Cluster age
character*1 u_AgeCluster ! Uncertainty flag on AgeCluster
character*1 l_AgeField ! Limit flag on AgeField
real*4 AgeField ! (Gyr) ? Field age
character*1 n_AgeField ! [a] Note on AgeField (2)
real*4 E_B_V ! (mag) Galactic reddening
real*4 v_Fe_H_C ! ([Sun]) ? This paper cluster metallicity
character*1 u__Fe_H_C ! Uncertainty flag on [Fe/H]C
real*4 v_Fe_H_O ! ([Sun]) ? Olszewski et al. (1991AJ....101..515O)
* cluster metallicity
character*1 u__Fe_H_O ! Uncertainty flag on [Fe/H]O
real*4 v_Fe_H_F ! ([Sun]) ? Field metallicity
character*1 u__Fe_H_F ! Uncertainty flag on [Fe/H]F
*Note (1): the letter has the following meaning:
* a: IC 2134 and SL 451 are located in the same frame
* b: SL 769 is included for comparison purposes: its location
* corresponds to the inner disk, i.e., in our definition when the
* mean field turnoff becomes as bright as the clump.
* This occurs at R~4{deg} (see text).
* The younger field turnoff are younger than intermediate age (<1Gyr)
* and outside of our age calibration.
* c: The field population corresponds essentially to that of the Galaxy
*Note (2): ameans that a significant fraction of younger stars is present.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! Washington photometry
integer*4 nr__1
parameter (nr__1=1788) ! Number of records
character*76 ar__1 ! Full-size record
character*12 Cluster_1 ! Cluster name
integer*4 ID ! Identification number in the cluster
real*8 Xpos ! (pix) X position (1)
real*8 Ypos ! (pix) Y position (1)
real*4 T1 ! (mag) T_1_ magnitude
real*4 e_T1 ! (mag) rms uncertainty on T1
real*4 C_T1 ! (mag) C-T_1_ colour index
real*4 e_C_T1 ! (mag) rms uncertainty on C-T1
real*4 CHI ! {chi} PARAMETER
real*4 SHARP ! SHARP parameter
*Note (1): 1 pix = 0.40". North is up, east is to the left.
C=============================================================================
C Loading file 'tab134.dat' ! Sample of outlying clusters and surrounding
* fields, ages, reddenings and metallicities
C Format for file interpretation
1 format(
+ A12,1X,A14,2X,I2,1X,I2,1X,I2,1X,A1,I2,1X,I2,1X,I2,1X,F5.1,1X,
+ F5.1,1X,F4.1,1X,F4.1,1X,A1,1X,F3.1,A1,1X,A1,F3.1,A1,1X,F4.2,
+ 1X,F5.2,A1,1X,F5.2,A1,1X,F5.2,A1)
C Effective file loading
open(unit=1,status='old',file=
+'tab134.dat')
write(6,*) '....Loading file: tab134.dat'
do i__=1,14
read(1,'(A108)')ar__
read(ar__,1)
+ Cluster,OtherName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,GLON,GLAT,Rad,R,
+ Note,AgeCluster,u_AgeCluster,l_AgeField,AgeField,n_AgeField,
+ E_B_V,v_Fe_H_C,u__Fe_H_C,v_Fe_H_O,u__Fe_H_O,v_Fe_H_F,u__Fe_H_F
if(ar__(79:81) .EQ. '') AgeField = rNULL__
if(ar__(89:93) .EQ. '') v_Fe_H_C = rNULL__
if(ar__(96:100) .EQ. '') v_Fe_H_O = rNULL__
if(ar__(103:107) .EQ. '') v_Fe_H_F = rNULL__
RAdeg = rNULL__
DEdeg = rNULL__
c Derive coordinates RAdeg and DEdeg from input data
c (RAdeg and DEdeg are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg=RAh*15.
if(RAm .GT. -180) RAdeg=RAdeg+RAm/4.
if(RAs .GT. -180) RAdeg=RAdeg+RAs/240.
if(DEd .GE. 0) DEdeg=DEd
if(DEm .GE. 0) DEdeg=DEdeg+DEm/60.
if(DEs .GE. 0) DEdeg=DEdeg+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg.GE.0) DEdeg=-DEdeg
c ..............Just test output...........
write(6,1)
+ Cluster,OtherName,RAh,RAm,RAs,DE_,DEd,DEm,DEs,GLON,GLAT,Rad,R,
+ Note,AgeCluster,u_AgeCluster,l_AgeField,AgeField,n_AgeField,
+ E_B_V,v_Fe_H_C,u__Fe_H_C,v_Fe_H_O,u__Fe_H_O,v_Fe_H_F,u__Fe_H_F
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table2.dat' ! Washington photometry
C Format for file interpretation
2 format(
+ A12,1X,I5,1X,F9.3,1X,F8.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,
+ F5.3,1X,F6.3)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,1788
read(1,'(A76)')ar__1
read(ar__1,2)
+ Cluster_1,ID,Xpos,Ypos,T1,e_T1,C_T1,e_C_T1,CHI,SHARP
c ..............Just test output...........
write(6,2)
+ Cluster_1,ID,Xpos,Ypos,T1,e_T1,C_T1,e_C_T1,CHI,SHARP
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end