FORTRAN Generation
(/./ftp/cats/J/ApJ/640/603)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/640/603 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-20
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/640/603      Catalog of AGNs in the GOODS fields         (Treister+, 2006)
*================================================================================
*Spitzer number counts of active galactic nuclei in the GOODS fields.
*    Treister E., Urry C.M., Van Duyne J., Dickinson M., Chary R.-R.,
*    Alexander D.M., Bauer F., Natarajan P., Lira P., Grogin N.A.
*   <Astrophys. J., 640, 603-611 (2006)>
*   =2006ApJ...640..603T
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Catalog of AGNs in the GOODS fields

      integer*4 nr__
      parameter (nr__=315)	! Number of records
      character*83 ar__   	! Full-size record

      character*1   F          (nr__) ! [NS] North or South field
      integer*4     v_ABB2003_ (nr__) ! ID from Alexander et al. (2003,
*                                  Cat. <J/AJ/126/539>)
      real*4        Prob       (nr__) ! Probability of random X-ray/IR association (1)
      real*4        Fsoft      (nr__) ! (mW/m2) Soft X-ray (0.5-2keV) flux (2)
      real*4        Fhard      (nr__) ! (mW/m2) Hard X-ray (2-8keV) flux (2)
      real*4        HR         (nr__) ! Hardness Ratio (3)
      real*4        F3_6um     (nr__) ! (uJy) The 3.6{mu}m flux
      real*4        F4_5um     (nr__) ! (uJy) The 4.5{mu}m flux
      real*4        F5_7um     (nr__) ! (uJy) The 5.7{mu}m flux
      real*8        F8um       (nr__) ! (uJy) The 8{mu}m flux
      real*8        F24um      (nr__) ! (uJy) The 24{mu}m flux
      real*4        z          (nr__) ! Redshift
      character*1   zType      (nr__) ! [SPN] Redshift type (4)
      character*1   Class      (nr__) ! Optical classification (5)
*Note (1): Probability of random association assuming a Poissonian
*          distribution of sources. Expression 1-exp(-n{pi}d^2^) was used
*          where n is the density of sources and d is the distance between
*          the X-ray and infrared sources.
*Note (2): In units of erg/cm^2^/s.
*Note (3): Defined as (H-S)/(H+S) where H and S are the background-substracted
*          counts in the Hard and Soft X-ray bands respectively.
*Note (4): Redshift type, defined as follows:
*      S = Spectroscopic Redshift;
*      P = Photometric Redshift;
*      N = No redshift measured.
*Note (5): Optical classification, defined as follows:
*      B = Broad line AGN;
*      N = Narrow line AGN;
*      G = Galaxy;
*      U = Unknown.

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

C  Loading file 'table1.dat'	! Catalog of AGNs in the GOODS fields

C  Format for file interpretation

    1 format(
     +  A1,1X,I3,1X,F5.3,1X,E9.2,1X,E8.2,1X,F5.2,1X,F6.2,1X,F6.2,1X,
     +  F6.2,1X,F7.2,1X,F7.2,1X,F5.3,1X,A1,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,315
        read(1,'(A83)')ar__
        read(ar__,1)
     +  F(i__),v_ABB2003_(i__),Prob(i__),Fsoft(i__),Fhard(i__),
     +  HR(i__),F3_6um(i__),F4_5um(i__),F5_7um(i__),F8um(i__),
     +  F24um(i__),z(i__),zType(i__),Class(i__)
c    ..............Just test output...........
        write(6,1)
     +  F(i__),v_ABB2003_(i__),Prob(i__),Fsoft(i__),Fhard(i__),
     +  HR(i__),F3_6um(i__),F4_5um(i__),F5_7um(i__),F8um(i__),
     +  F24um(i__),z(i__),zType(i__),Class(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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