Conversion of standardized ReadMe file for
file /./ftp/cats/J/MNRAS/382/1342 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/MNRAS/382/1342 Compact stellar systems around NGC 1399 (Firth+, 2007)
*================================================================================
*Compact stellar systems around NGC 1399.
* Firth P., Drinkwater M.J., Evstigneeva E.A., Gregg M.D., Karick A.M.,
* Jones J.B., Phillipps S.
* <Mon. Not. R. Astron. Soc., 382, 1342-1352 (2007)>
* =2007MNRAS.382.1342F (SIMBAD/NED BibCode)
C=============================================================================
C Internal variables
integer*4 i__
c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -
C Declarations for 'table2.dat' ! *Bound and unbound compact stellar systems (CSS)
integer*4 nr__
parameter (nr__=63) ! Number of records
character*108 ar__ ! Full-size record
C J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
real*8 RAdeg ! (deg) Right Ascension J2000
real*8 DEdeg ! (deg) Declination J2000
C ---------------------------------- ! (position vector(s) in degrees)
integer*4 Type ! [1/3] Type of cluster (1)
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)
real*4 g_mag ! (mag) Deredenned CTIO g' magnitude
real*4 r_mag ! (mag) Deredenned CTIO r' magnitude
real*4 i_mag ! (mag) Deredenned CTIO i' magnitude
real*4 SGC_r ! Stellarity index (2)
character*1 n_SGC_r ! [cde] Note on SGC-r (3)
integer*4 cz1 ! (km/s) ? 2dF heliocentric recessional velocity (4)
integer*4 e_cz1 ! (km/s) ? rms uncertainty on cz1
integer*4 cz2 ! (km/s) ? FCOS heliocentric recessional velocity (5)
integer*4 e_cz2 ! (km/s) ? rms uncertainty on cz2
integer*4 cz3 ! (km/s) ? Bergond heliocentric recessional velocity (6)
integer*4 e_cz3 ! (km/s) ? rms uncertainty on cz3
integer*4 cz4 ! (km/s) ? VLT-FLAMES heliocentric recessional velocity
integer*4 e_cz4 ! (km/s) ? rms uncertainty on cz4
real*4 R ! ? VLT-FLAMES cross-correlation R value
character*1 n_R ! [)] ) indicates value from the previously
* published redshift measurement with the
* lowest error margin
character*11 Galaxy ! Associated galaxy name
real*4 DV_V ! ? Ratio of the recessional velocity difference
* (between the CSS and its potentially
* associated galaxy) and the escape velocity at
* the projected radius (7)
character*1 n_DV_V ! [a] bound to a prominent cluster (8)
*Note (1): Type of cluster as follows:
* 1 = known Fornax cluster galaxies
* 2 = known Fornax cluster compact stellar systems (CSS)
* 3 = new Fornax cluster compact stellar systems (CSS)
*Note (2): The stellarity index (SGC-r), derived by SExtractor from r' band
* photometry (Karick, 2005, PhD thesis, Univ. Melbourne), compares the
* target light profile to a point-spread function (0 = extended object;
* 1 = point source)
*Note (3): Note on SGC-r as follows:
* c = Photometry of these CSS has been affected by partial blending
* with adjacent stars.
* d = UCD3 is known to have an extended stellar halo (De Propris et al.
* 2005ApJ...623L.105D), and may be eventually classified as a
* dE,N galaxy (see full version of table).
* e = Photometry of this CSS has been affected by blending with a
* background galaxy
*Note (4): 2dF revised velocity data are derived from Drinkwater et al.
* (2000PASA...17..227D) and Gregg (in preparation).
*Note (5): FCOS data are from the Fornax Compact Object Survey (Mieske et
* al., 2004, Cat. J/A+A/418/445). FCOS catalogue identifiers (as
* sequenced in the table): 1-017, 2-0231, 2-078, 4-2028, 2-073, 0-2025,
* 3-2027, 1-2053, 1-060, 3-2004, 1-2083 and 3-2019.
*Note (6): Bergond data are from VLT-FLAMES spectroscopy (Bergond et al.,
* 2006, Cat. J/A+A/448/155).
*Note (7): Therefore, a ratio less than 1 implies they are gravitationally
* bound.
*Note (8): 'a' quotes CSS considered to be gravitationally bound to a
* prominent cluster galaxy other than NGC 1399 - see analysis in
* the text.
C=============================================================================
C Loading file 'table2.dat' ! *Bound and unbound compact stellar systems (CSS)
C Format for file interpretation
1 format(
+ I1,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F5.2,1X,F5.2,
+ 1X,F5.2,1X,F4.2,A1,1X,I4,1X,I3,1X,I4,1X,I3,1X,I4,1X,I3,1X,I4,
+ 1X,I2,1X,F5.2,A1,1X,A11,1X,F3.1,A1)
C Effective file loading
open(unit=1,status='old',file=
+'table2.dat')
write(6,*) '....Loading file: table2.dat'
do i__=1,63
read(1,'(A108)')ar__
read(ar__,1)
+ Type,RAh,RAm,RAs,DE_,DEd,DEm,DEs,g_mag,r_mag,i_mag,SGC_r,
+ n_SGC_r,cz1,e_cz1,cz2,e_cz2,cz3,e_cz3,cz4,e_cz4,R,n_R,Galaxy,
+ DV_V,n_DV_V
if(ar__(51:54) .EQ. '') cz1 = iNULL__
if(ar__(56:58) .EQ. '') e_cz1 = iNULL__
if(ar__(60:63) .EQ. '') cz2 = iNULL__
if(ar__(65:67) .EQ. '') e_cz2 = iNULL__
if(ar__(69:72) .EQ. '') cz3 = iNULL__
if(ar__(74:76) .EQ. '') e_cz3 = iNULL__
if(ar__(78:81) .EQ. '') cz4 = iNULL__
if(ar__(83:84) .EQ. '') e_cz4 = iNULL__
if(ar__(86:90) .EQ. '') R = rNULL__
if(ar__(105:107) .EQ. '') DV_V = 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)
+ Type,RAh,RAm,RAs,DE_,DEd,DEm,DEs,g_mag,r_mag,i_mag,SGC_r,
+ n_SGC_r,cz1,e_cz1,cz2,e_cz2,cz3,e_cz3,cz4,e_cz4,R,n_R,Galaxy,
+ DV_V,n_DV_V
write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c .......End.of.Just test output...........
end do
close(1)
C=============================================================================
stop
end