Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/402/1729 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/MNRAS/402/1729 JHK photometry of 36 Galactic globular clusters (Valenti+ 2010)
*================================================================================
*Near-infrared properties of 12 globular clusters towards the inner bulge
*of the galaxy.
* Valenti E., Ferraro F.R., Origlia L.
* <Mon. Not. R. Astron. Soc., 402, 1729-1739 (2010)>
* =2010MNRAS.402.1729V
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table1.dat' ! The Bulge Globular Cluster parameters for
all clusters (Paper I + Paper II)
integer*4 nr__
parameter (nr__=36) ! Number of records
character*166 ar__ ! Full-size record
C Position composed of: GLON GLAT
character*7 GlCl ! Globular name
character*1 n_GlCl ! [*] Note on Name (1)
real*4 GLON ! (deg) [-15/21] Galactic longitude
real*4 GLAT ! (deg) Galactic latitude
real*4 dSun ! (kpc) Heliocentric distance
real*4 RGC ! (kpc) Galactocentric distance
real*4 X ! (kpc) X Sun-centred coordinate
real*4 Y ! (kpc) Y Sun-centred coordinate
real*4 Z ! (kpc) Z Sun-centred coordinate
real*4 E_B_V ! (mag) B-V colour excess
real*4 v_m_M_0 ! (mag) Deredenned distance modulus
real*4 v_Fe_H_ ! ([-]) Metallicity [Fe/H] (2)
real*4 v_M_H_ ! ([-]) Metallicity [M/H]
real*4 JRC ! (mag) ?=- Horizontal Branch Red Clump J magnitude
real*4 HRC ! (mag) ?=- Horizontal Branch Red Clump H magnitude
real*4 KsRC ! (mag) ?=- Horizontal Branch Red Clump Ks magnitude
real*4 Jmag_B ! (mag) ?=- Bump J magnitude
real*4 Hmag_B ! (mag) ?=- Bump H magnitude
real*4 Kmag_B ! (mag) ?=- Bump Ks magnitude
real*4 Jmag_T ! (mag) Tip J magnitude
real*4 Hmag_T ! (mag) ?=- Tip H magnitude
real*4 Kmag_T ! (mag) ?=- Tip Ks magnitude
real*4 Mbol_B ! (mag) ?=- RGB Bump bolometric magnitude (3)
real*4 Mbol_T ! (mag) ?=- Tip bolometric magnitude (3)
character*12 CMD ! Name of the file containing the CMD,
* at http://www.bo.astro.it/~GC/ir_archive/
integer*4 N ! Number of stars with photometry in FileName
character*11 FileName ! Name of the file containing the JHK photometry,
* in subdirectory phot
*Note (1): For all the clusters marked with (*) the metallicity estimates
* ([Fe/H] and [M/H]) have been derived by using the empirical method of
* Ferraro, Valenti & Origlia (2006ApJ...649..243F; see also IR relations
* at http://www.bo.astro.it/~GC/ir_archive/IRrelations.html)
*Note (2): [Fe/H] is in the Carretta & Gratton (1997, J/A+AS/121/95) scale.
*Note (3): The Bolometric magnitudes of the RGB Bump and Tip have been
* derived by using the bolometric corrections for Population II giants
* computed by Montegriffo et al. (1998MNRAS.297..872M), and by adopting
* the reddening and distance values listed in Table 1 and the extinction
* coefficients of Savage & Mathis (1979ARA&A..17...73S).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'phot/*' ! Individual JHK photometry
integer*4 nr__1
parameter (nr__1=36) ! Number of records
character*67 ar__1 ! Full-size record
C J2000 position composed of: RAdeg DEdeg
integer*4 Seq ! Sequential number within the cluster (1)
real*4 Jmag ! (mag) ?=0.000 SOFI J magnitude
real*4 Hmag ! (mag) ? (?=0.000) SOFI H magnitude
real*4 Kmag ! (mag) ? (?=0.000) SOFI Ks magnitude
real*8 RAdeg ! (deg) Right ascension in decimal degrees (J2000)
real*8 DEdeg ! (deg) Declination in decimal degrees (J2000)
*Note (1): Stars are identified as:
* Cl* NGC NNNN VFO NNNNN for NGC clusters,
* Cl* TERZAN N VFO NNNNN for Terzan clusters,
* Cl* HP 1 VFO NNNNN for HP1 cluster,
* Cl* Liller 1 VFO NNNNN for Liller1 cluster,
* Cl* Djorg N VFO NNNNN for Djorg clusters.
C=============================================================================
C Loading file 'table1.dat' ! The Bulge Globular Cluster parameters for
* all clusters (Paper I + Paper II)
C Format for file interpretation
1 format(
+ A7,A1,1X,F6.2,1X,F6.2,1X,F4.1,1X,F3.1,1X,F4.1,1X,F4.1,1X,F5.2,
+ F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,
+ 1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,
+ A12,1X,I5,1X,A11)
C Effective file loading
open(unit=1,status='old',file=
+'table1.dat')
write(6,*) '....Loading file: table1.dat'
do i__=1,36
read(1,'(A166)')ar__
read(ar__,1)
+ GlCl,n_GlCl,GLON,GLAT,dSun,RGC,X,Y,Z,E_B_V,v_m_M_0,v_Fe_H_,
+ v_M_H_,JRC,HRC,KsRC,Jmag_B,Hmag_B,Kmag_B,Jmag_T,Hmag_T,Kmag_T,
+ Mbol_B,Mbol_T,CMD,N,FileName
if (idig(ar__(72:76)).EQ.0) JRC = rNULL__
if (idig(ar__(78:82)).EQ.0) HRC = rNULL__
if (idig(ar__(84:88)).EQ.0) KsRC = rNULL__
if (idig(ar__(90:94)).EQ.0) Jmag_B = rNULL__
if (idig(ar__(96:100)).EQ.0) Hmag_B = rNULL__
if (idig(ar__(102:106)).EQ.0) Kmag_B = rNULL__
if (idig(ar__(114:118)).EQ.0) Hmag_T = rNULL__
if (idig(ar__(120:124)).EQ.0) Kmag_T = rNULL__
if (idig(ar__(126:129)).EQ.0) Mbol_B = rNULL__
if (idig(ar__(131:135)).EQ.0) Mbol_T = rNULL__
c ..............Just test output...........
write(6,1)
+ GlCl,n_GlCl,GLON,GLAT,dSun,RGC,X,Y,Z,E_B_V,v_m_M_0,v_Fe_H_,
+ v_M_H_,JRC,HRC,KsRC,Jmag_B,Hmag_B,Kmag_B,Jmag_T,Hmag_T,Kmag_T,
+ Mbol_B,Mbol_T,CMD,N,FileName
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'phot/*' ! Individual JHK photometry
C Format for file interpretation
2 format(3X,I5,3X,F6.3,3X,F6.3,3X,F6.3,4X,F13.9,2X,F13.9)
C Effective file loading
open(unit=1,status='old',file=
+'phot/*')
write(6,*) '....Loading file: phot/*'
do i__=1,36
read(1,'(A67)')ar__1
read(ar__1,2)Seq,Jmag,Hmag,Kmag,RAdeg,DEdeg
if(ar__1(21:26) .EQ. '') Hmag = rNULL__
if(ar__1(30:35) .EQ. '') Kmag = rNULL__
c ..............Just test output...........
write(6,2)Seq,Jmag,Hmag,Kmag,RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end
C Locate position of first digit in string; or return 0
integer function idig(c)
character*(*) c
character*1 c1
integer lc,i
lc=len(c)
idig=0
do i=1,lc
if(c(i:i).ne.' ') go to 1
end do
1 if(i.gt.lc) return
c1=c(i:i)
if(c1.eq.'.'.or.c1.eq.'-'.or.c1.eq.'+') i=i+1
if(i.gt.lc) return
c1=c(i:i)
if(c1.ge.'0'.and.c1.le.'9') idig=i
return
end