Conversion of standardized ReadMe file for
file /./ftp/cats/J/ApJ/789/115 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-19
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/ApJ/789/115 The Quintuplet cluster astrometry and photometry (Stolte+, 2014)
*================================================================================
*The orbital motion of the Quintuplet cluster - A common origin for the Arches
*and Quintuplet clusters?
* Stolte A., Hussmann B., Morris M.R., Ghez A.M., Brandner W., Lu J.R.,
* Clarkson W.I., Habibi M., Matthews K.
* <Astrophys. J., 789, 115 (2014)>
* =2014ApJ...789..115S (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table3.dat' ! Astrometry & photometry of NACO 2003
& NIRC2 2008 & 2009 sources
integer*4 nr__
parameter (nr__=226) ! Number of records
character*97 ar__ ! Full-size record
integer*4 Seq ! Sequential number
real*4 dRA ! (arcsec) Right Ascension offset (J2000) (G1)
real*4 dDE ! (arcsec) Declination offset (J2000) (G1)
real*8 pmRA ! (mas/yr) Proper motion in RA; milliarcsec/yr
real*4 e_pmRA ! (mas/yr) Uncertainty in pmRA
real*8 pmDE ! (mas/yr) Proper motion in Declination; milliarcsec/yr
real*4 e_pmDE ! (mas/yr) Uncertainty in pmDE
real*4 Kmag09 ! (mag) The 2009 Keck/NIRC2 K' band magnitude (G2)
real*4 e_Kmag09 ! (mag) Uncertainty in Kmag09
real*8 Kmag08 ! (mag) ?=-99.99 The 2008 Keck/NIRC2 K' band
* magnitude (G2)
real*8 e_Kmag08 ! (mag) ?=-99.99 Uncertainty in Kmag08
real*4 Kmag03 ! (mag) The 2003 VLT/NAOS-CONICA K_s_ band
* magnitude (G2)
real*4 e_Kmag03 ! (mag) Uncertainty in Kmag03
real*8 pclus ! ?=-99.99 Membership probability indicator (3)
*Note (3): For stars deviating significantly from the cluster and field
* distributions, the membership probability could not be determined.
* pclus has a value of -99.99 in these cases. Monte Carlo simulations
* of the proper motion plane for one of the outer cluster fields (the
* Pistol field, Field 2 in Hussmann 2014, PhD thesis, Univ. Bonn,
* http://www.astro.uni-bonn.de/~hussmann/thesis/) suggest that cluster
* and field stars are most efficiently separated with a formal
* probability threshold of pclus > 0.4 (see Sections 4.2.2.1 to
* 4.2.2.3 in Hussmann (2014) for details).
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table4.dat' ! Astrometry & photometry of NACO 2003
& NACO 2008 sources
integer*4 nr__1
parameter (nr__1=2137) ! Number of records
character*82 ar__1 ! Full-size record
integer*4 Seq_1 ! Sequential number
real*8 dRA_1 ! (arcsec) Right Ascension offset (J2000) (G1)
real*8 dDE_1 ! (arcsec) Declination offset (J2000) (G1)
real*8 pmRA_1 ! (mas/yr) Proper motion in RA; milliarcsec/yr
real*4 e_pmRA_1 ! (mas/yr) Uncertainty in pmRA
real*8 pmDE_1 ! (mas/yr) Proper motion in Declination; milliarcsec/yr
real*4 e_pmDE_1 ! (mas/yr) Uncertainty in pmDE
real*4 Kmag03_1 ! (mag) The 2003 VLT/NACO K_s_ band magnitude (G2)
real*4 e_Kmag03_1 ! (mag) Uncertainty in Kmag03
real*4 Kmag08_1 ! (mag) The 2008 VLT/NACO K_S_ band magnitude (G2)
real*4 e_Kmag08_1 ! (mag) Uncertainty in Kmag08
real*8 pclus_1 ! ?=-99.99 Membership probability indicator (3)
*Note (3): For stars deviating significantly from the cluster and field
* distributions, the membership probability could not be determined.
* pclus has a value of -99.99 in these cases.
C=============================================================================
C Loading file 'table3.dat' ! Astrometry & photometry of NACO 2003
* & NIRC2 2008 & 2009 sources
C Format for file interpretation
1 format(
+ I3,1X,F6.3,1X,F6.3,1X,F7.4,1X,F6.4,1X,F7.4,1X,F6.4,1X,F6.3,1X,
+ F5.3,1X,F7.3,1X,F7.3,1X,F6.3,1X,F5.3,1X,F7.3)
C Effective file loading
open(unit=1,status='old',file=
+'table3.dat')
write(6,*) '....Loading file: table3.dat'
do i__=1,226
read(1,'(A97)')ar__
read(ar__,1)
+ Seq,dRA,dDE,pmRA,e_pmRA,pmDE,e_pmDE,Kmag09,e_Kmag09,Kmag08,
+ e_Kmag08,Kmag03,e_Kmag03,pclus
c ..............Just test output...........
write(6,1)
+ Seq,dRA,dDE,pmRA,e_pmRA,pmDE,e_pmDE,Kmag09,e_Kmag09,Kmag08,
+ e_Kmag08,Kmag03,e_Kmag03,pclus
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'table4.dat' ! Astrometry & photometry of NACO 2003
* & NACO 2008 sources
C Format for file interpretation
2 format(
+ I4,1X,F7.3,1X,F7.3,1X,F7.3,1X,F5.3,1X,F7.3,1X,F5.3,1X,F6.3,1X,
+ F5.3,1X,F6.3,1X,F5.3,1X,F7.3)
C Effective file loading
open(unit=1,status='old',file=
+'table4.dat')
write(6,*) '....Loading file: table4.dat'
do i__=1,2137
read(1,'(A82)')ar__1
read(ar__1,2)
+ Seq_1,dRA_1,dDE_1,pmRA_1,e_pmRA_1,pmDE_1,e_pmDE_1,Kmag03_1,
+ e_Kmag03_1,Kmag08_1,e_Kmag08_1,pclus_1
c ..............Just test output...........
write(6,2)
+ Seq_1,dRA_1,dDE_1,pmRA_1,e_pmRA_1,pmDE_1,e_pmDE_1,Kmag03_1,
+ e_Kmag03_1,Kmag08_1,e_Kmag08_1,pclus_1
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end