FORTRAN Generation
(/./ftp/cats/J/AJ/130/968)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AJ/130/968 into FORTRAN code for loading all data files into arrays.

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/AJ/130/968         SDSS-C4 cluster catalog                     (Miller+, 2005)
*================================================================================
*The C4 clustering algorithm: clusters of galaxies in the Sloan Digital Sky
*Survey.
*    Miller C.J., Nichol R.C., Reichart D., Wechsler R.H., Evrard A.E.,
*    Annis J., McKay T.A., Bahcall N.A., Bernardi M., Boehringer H.,
*    Connolly A.J., Goto T., Kniazev A., Lamb D., Postman M., Schneider D.P.,
*    Sheth R.K., Voges W.
*   <Astron. J., 130, 968-1001 (2005)>
*   =2005AJ....130..968M
C=============================================================================

C  Internal variables

      integer*4 i__

c - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - 

C  Declarations for 'table2.dat'	! The SDSS-C4 cluster catalog (DR2)

      integer*4 nr__
      parameter (nr__=748)	! Number of records
      character*147 ar__   	! Full-size record

C  J2000 position composed of: RA1deg DE1deg
      integer*4     SDSS_C4    (nr__) ! Source SDSS C4 identification
      real*8        RA1deg     (nr__) ! (deg) Right Ascension from Method 1 (J2000) (1)
      real*8        DE1deg     (nr__) ! (deg) Declination from Method 1 (J2000) (1)
      real*8        RA2deg     (nr__) ! (deg) Right Ascension from Method 2 (J2000) (1)
      real*8        DE2deg     (nr__) ! (deg) Declination from Method 2 (J2000) (1)
      real*8        RAbdeg     (nr__) ! (deg) Right Ascension of Brightest galaxy (J2000) (1)
      real*8        DEbdeg     (nr__) ! (deg) Declination of Brightest galaxy (J2000) (1)
      real*8        z          (nr__) ! Mean cluster redshift
      integer*4     sigma      (nr__) ! (km/s) Velocity dispersion (2)
      integer*4     Rich       (nr__) ! Richness
      real*4        Lr         (nr__) ! (solLum) Summed r-band cluster luminosity (3)
      integer*4     SCF        (nr__) ! [0,2] Structure Contamination Flag (4)
      real*4        DS         (nr__) ! Dressler-Shectman substructure statistics (a low
*                                 value indicates a significant substructure)
      character*50  ONames     (nr__) ! Other names (5)
*Note (1): In decimal degrees. Method 1 uses the peak in the C4 density field as
*          cluster centroid. Method 2 uses the luminosity-weighted mean centroid.
*Note (2): To convert to the rest-frame of the cluster, divide by 1+z.
*Note (3): Corrected for missed targets.
*Note (4): We define a "structure contamination flag" (SCF) to measure the degree
*          of isolation in redshift space for each cluster. We assign an SCF
*          based on the ratio of the standard deviation of the dispersions over
*          the mean of the velocity dispersions. A cluster with SCF=0 has a ratio
*          of less than 15%, whereas SCF=2 has a ratio >30%.
*Note (5): Matched to within 10 arcminute of the cluster centroid.

C=============================================================================

C  Loading file 'table2.dat'	! The SDSS-C4 cluster catalog (DR2)

C  Format for file interpretation

    1 format(
     +  I4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F8.4,1X,F7.5,1X,
     +  I4,1X,I3,1X,E12.6,1X,I1,1X,F4.2,1X,A50)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,748
        read(1,'(A147)')ar__
        read(ar__,1)
     +  SDSS_C4(i__),RA1deg(i__),DE1deg(i__),RA2deg(i__),DE2deg(i__),
     +  RAbdeg(i__),DEbdeg(i__),z(i__),sigma(i__),Rich(i__),Lr(i__),
     +  SCF(i__),DS(i__),ONames(i__)
c    ..............Just test output...........
        write(6,1)
     +  SDSS_C4(i__),RA1deg(i__),DE1deg(i__),RA2deg(i__),DE2deg(i__),
     +  RAbdeg(i__),DEbdeg(i__),z(i__),sigma(i__),Rich(i__),Lr(i__),
     +  SCF(i__),DS(i__),ONames(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

C=============================================================================
      stop
      end