Conversion of standardized ReadMe file for
file /./ftp/cats/J/A_A/618/A2 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 2026-Aug-15
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+A/618/A2 Quintuplet cluster updated stellar census (Clark+, 2018)
*================================================================================
*An updated stellar census of the Quintuplet cluster.
* Clark J.S., Lohr M.E., Patrick L.R., Najarro F., Dong H., Figer D.F.
* <Astron. Astrophys., 618, A2 (2018)>
* =2018A&A...618A...2C (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea1.dat' ! HST photometry of stellar members of the
Quintuplet cluster
integer*4 nr__
parameter (nr__=108) ! Number of records
character*101 ar__ ! Full-size record
C J2000 position composed of: RAdeg DEdeg
character*11 ID ! qF number or other name (1)
integer*4 LHO ! ?=- LHO number
real*8 RAdeg ! (deg) Right ascension (J2000)
real*8 DEdeg ! (deg) Declination (J2000)
real*4 F110W ! (mag) ?=- HST F110W magnitude
real*4 e_F110W ! (mag) ? rms uncertainty on F110W
character*1 n_F110W ! [*] Uncertainty flag on F110W
real*4 F160W ! (mag) ?=- HST F160W magnitude
real*4 e_F160W ! (mag) ? rms uncertainty on F160W
character*1 n_F160W ! [*] Uncertainty flag on F160W
real*4 F205W ! (mag) ?=- HST F205W magnitude
real*4 e_F205W ! (mag) ? rms uncertainty on F205W
character*1 n_F205W ! [*] Uncertainty flag on F205W
real*4 F127M ! (mag) ?=- HST F127M magnitude
real*4 e_F127M ! (mag) ? rms uncertainty on F127M
real*4 F139M ! (mag) ?=- HST F139M magnitude
real*4 e_F139M ! (mag) ? rms uncertainty on F139M
real*4 F153M ! (mag) ?=- HST F153M magnitude
real*4 e_F153M ! (mag) ? rms uncertainty on F153M
*Note (1): Objects for which no photometry is available are
* qF76 (WC9; this work),
* qF269 (OB I; Figer at al., 1999ApJ...514..202F),
* qF301 (< OB I; Figer at al., 1999ApJ...514..202F),
* qF311 (B1-3 I; Figer at al., 1999ApJ...514..202F),
* qF362 (LBV; Geballe et al., 2000ApJ...530L..97G),
* LHO23 (O3-6 I-II; Liermann et al., 2009, Cat. J/A+A/494/1137),
* LHO70 (O7-8 If; Liermann et al., 2009, Cat. J/A+A/494/1137) and
* G0.120-0.048 (LBV; Mauerhan et al. 2010ApJ...710..706M).
*
* qF353E, qF381 and qF406 were outside the NICMOS field-of-view and hence lack
* F110W, F160W and F205W magnitudes.
*
* The following sources had multiple counterparts within 2.5 pixels of their
* position in the NICMOS data;
* qF276 (two sources with one 2.5mag fainter; brighter selected),
* LHO15 (two sources with a difference of 0.3m; closest selected),
* LHO64 (two sources with one 3.4mag fainter; brighter selected),
* LHO72 (two sources with one 1.2mag fainter; closest selected) and
* LHO73 (two sources within one pixel with broadly comparable magnitudes;
* closest selected).
*
* Caution should therefore be applied regarding the F110W, F160W and F205W
* magnitudes for LHO15, LHO72 and LHO73; these are followed by an *.
*
* Finally no NICMOS counterpart to LHO139 was found within 9 pixels of the
* anticipated position.
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'tablea2.dat' ! Stellar population of the Quintuplet cluster
integer*4 nr__1
parameter (nr__1=71) ! Number of records
character*112 ar__1 ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg_1 ! (deg) Right Ascension J2000
real*8 DEdeg_1 ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
character*12 ID_1 ! qF number or other name (G1)
integer*4 LHO_1 ! ? LHO number (G2)
integer*4 RAh ! (h) Right ascension (J2000)
integer*4 RAm ! (min) Right ascension (J2000)
real*4 RAs ! (s) Right ascension (J2000)
character*1 DE_ ! Declination sign (J2000)
integer*4 DEd ! (deg) Declination (J2000)
integer*4 DEm ! (arcmin) Declination (J2000)
real*4 DEs ! (arcsec) Declination (J2000)
character*16 ClassC ! Most up-to-date spectral classification
* available from either Figer at al.
* (1999ApJ...514..202F) or Liermann et al.,
* 2009, Cat. J/A+A/494/1137)
character*14 ClassR ! Revised classification, this paper
character*39 Notes ! Notes (1)
*Note (1): additional widely used identifiers (e.g. WR number and the naming
* convention of Dong et al., 2011, Cat. J/MNRAS/417/114).
* qF309 and qF344 are re-classified via comparison of the spectra from
* Figer at al. (1999ApJ...514..202F) and Mauerhan et al. (2010ApJ...710..706M)
* to our new data.
* The five Quintuplet proper members are those stars with MGM 5-# identifiers
* (Moneti et al. 1992MNRAS.258..705M).
* QX# and QR# indicate radio and X-ray detections reported in Lang et al.
* (2005AJ....130.2185L) and Wang et al. (2006MNRAS.371...38W) respectively.
* The Pistol star is also reported as a radio source but no new identifier is
* assigned for it, while the X-ray designation of qF344 derives from Muno et al.
* (2009, Cat. J/ApJS/181/110).
* Tuthill et al. (2006Sci...313..935T) provide the orbital period for qF211 and
* suggest periods in the hundreds of days for qF243, qF251, and qF258 based on
* the size of their dusty nebulae.
C=============================================================================
C Loading file 'tablea1.dat' ! HST photometry of stellar members of the
* Quintuplet cluster
C Format for file interpretation
1 format(
+ A11,1X,I3,1X,F9.5,1X,F9.5,1X,F5.2,1X,F4.2,A1,F5.2,1X,F4.2,A1,
+ F5.2,1X,F4.2,A1,F5.2,1X,F4.2,1X,F5.2,1X,F4.2,1X,F5.2,1X,F4.2)
C Effective file loading
open(unit=1,status='old',file=
+'tablea1.dat')
write(6,*) '....Loading file: tablea1.dat'
do i__=1,108
read(1,'(A101)')ar__
read(ar__,1)
+ ID,LHO,RAdeg,DEdeg,F110W,e_F110W,n_F110W,F160W,e_F160W,
+ n_F160W,F205W,e_F205W,n_F205W,F127M,e_F127M,F139M,e_F139M,
+ F153M,e_F153M
if (LHO .EQ. 45) LHO = iNULL__
if (idig(ar__(37:41)).EQ.0) F110W = rNULL__
if(ar__(43:46) .EQ. '') e_F110W = rNULL__
if (idig(ar__(48:52)).EQ.0) F160W = rNULL__
if(ar__(54:57) .EQ. '') e_F160W = rNULL__
if (idig(ar__(59:63)).EQ.0) F205W = rNULL__
if(ar__(65:68) .EQ. '') e_F205W = rNULL__
if (idig(ar__(70:74)).EQ.0) F127M = rNULL__
if(ar__(76:79) .EQ. '') e_F127M = rNULL__
if (idig(ar__(81:85)).EQ.0) F139M = rNULL__
if(ar__(87:90) .EQ. '') e_F139M = rNULL__
if (idig(ar__(92:96)).EQ.0) F153M = rNULL__
if(ar__(98:101) .EQ. '') e_F153M = rNULL__
c ..............Just test output...........
write(6,1)
+ ID,LHO,RAdeg,DEdeg,F110W,e_F110W,n_F110W,F160W,e_F160W,
+ n_F160W,F205W,e_F205W,n_F205W,F127M,e_F127M,F139M,e_F139M,
+ F153M,e_F153M
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
C Loading file 'tablea2.dat' ! Stellar population of the Quintuplet cluster
C Format for file interpretation
2 format(
+ A12,I3,2X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,A16,1X,
+ A14,1X,A39)
C Effective file loading
open(unit=1,status='old',file=
+'tablea2.dat')
write(6,*) '....Loading file: tablea2.dat'
do i__=1,71
read(1,'(A112)')ar__1
read(ar__1,2)
+ ID_1,LHO_1,RAh,RAm,RAs,DE_,DEd,DEm,DEs,ClassC,ClassR,Notes
if(ar__1(13:15) .EQ. '') LHO_1 = iNULL__
RAdeg_1 = rNULL__
DEdeg_1 = rNULL__
c Derive coordinates RAdeg_1 and DEdeg_1 from input data
c (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
if(RAh .GT. -180) RAdeg_1=RAh*15.
if(RAm .GT. -180) RAdeg_1=RAdeg_1+RAm/4.
if(RAs .GT. -180) RAdeg_1=RAdeg_1+RAs/240.
if(DEd .GE. 0) DEdeg_1=DEd
if(DEm .GE. 0) DEdeg_1=DEdeg_1+DEm/60.
if(DEs .GE. 0) DEdeg_1=DEdeg_1+DEs/3600.
if(DE_.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c ..............Just test output...........
write(6,2)
+ ID_1,LHO_1,RAh,RAm,RAs,DE_,DEd,DEm,DEs,ClassC,ClassR,Notes
write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
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