FORTRAN Generation
(/./ftp/cats/J/ApJ/559/606)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/559/606 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-16
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/559/606       Star formation in spectroscopic survey   (Carter+, 2001)
*================================================================================
*Star formation in a complete spectroscopic survey of galaxies.
*     Carter B.J., Fabricant D.G., Geller M.J., Kurtz M.J., McLean B.
*    <Astrophys. J. 559, 606 (2001)>
*    =2001ApJ...559..606C
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table3.dat'	! The Most Vigorous Star-Forming Galaxies in
                             the 15R Sample

      integer*4 nr__
      parameter (nr__=32)	! Number of records
      character*41 ar__   	! Full-size record

C  1950 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg      (nr__) ! (deg) Right Ascension 1950
      real*8        DEdeg      (nr__) ! (deg)     Declination 1950
C  ---------------------------------- ! (position vector(s) in degrees)

      integer*4     RAh        (nr__) ! (h) Right ascension (1950) (1)
      integer*4     RAm        (nr__) ! (min) Right ascension (1950)
      real*4        RAs        (nr__) ! (s) Right ascension (1950)
      character*1   DE_        (nr__) ! Declination sign (1950)
      integer*4     DEd        (nr__) ! (deg) Declination (1950)
      integer*4     DEm        (nr__) ! (arcmin) Declination (1950)
      real*4        DEs        (nr__) ! (arcsec) Declination (1950)
      character*1   Orient     (nr__) ! [ENSW] Orientation
      real*4        b          (nr__) ! Scalo stellar birthrate parameter (2)
      integer*4     cz         (nr__) ! (km/s) Heliocentric redshift
      real*4        EW_Halpha  (nr__) ! (0.1nm) H{alpha} equivalent width
*Note (1): Galaxies identified as [CFG2001] 15R HHMMSS.s+DDMMSS.s in Simbad
*Note (2): Scalo stellar birthrate parameter:
*    b = SFR/<SFR> = [(SFR*tau_d_)/M_d_]*(1-R_f_), where 
*      M_d_ is the stellar mass, 
*    tau_d_ is the age of the stellar population, and 
*      R_f_ is the fraction of mass in each stellar generation that is not 
*           tied up in stars (Tinsley, 1980, Fundam. Cosmic Phys., 5, 287)

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

C  Loading file 'table3.dat'	! The Most Vigorous Star-Forming Galaxies in
*                             the 15R Sample

C  Format for file interpretation

    1 format(
     +  I2,1X,I2,1X,F4.1,1X,A1,I2,1X,I2,1X,F4.1,1X,A1,1X,F4.1,1X,I5,
     +  1X,F5.1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,32
        read(1,'(A41)')ar__
        read(ar__,1)
     +  RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
     +  DEs(i__),Orient(i__),b(i__),cz(i__),EW_Halpha(i__)
        RAdeg(i__) = rNULL__
        DEdeg(i__) = rNULL__
c  Derive coordinates RAdeg and DEdeg from input data
c  (RAdeg and DEdeg are set to rNULL__ when unknown)
        if(RAh(i__) .GT. -180) RAdeg(i__)=RAh(i__)*15.
        if(RAm(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAm(i__)/4.
        if(RAs(i__) .GT. -180) RAdeg(i__)=RAdeg(i__)+RAs(i__)/240.
        if(DEd(i__) .GE. 0) DEdeg(i__)=DEd(i__)
        if(DEm(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEm(i__)/60.
        if(DEs(i__) .GE. 0) DEdeg(i__)=DEdeg(i__)+DEs(i__)/3600.
        if(DE_(i__).EQ.'-'.AND.DEdeg(i__).GE.0) DEdeg(i__)=-DEdeg(i__)
c    ..............Just test output...........
        write(6,1)
     +  RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),DEm(i__),
     +  DEs(i__),Orient(i__),b(i__),cz(i__),EW_Halpha(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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