FORTRAN Generation
(/./ftp/cats/J/ApJ/679/140)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/679/140 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-Mar-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/ApJ/679/140      IR measurement of quasar obscuration        (Treister+, 2008)
*================================================================================
*Measuring the fraction of obscured quasars by the infrared luminosity of
*unobscured quasars.
*    Treister E., Krolik J.H., Dullemond C.
*   <Astrophys. J., 679, 140-148 (2008)>
*   =2008ApJ...679..140T
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Observed properties of sources in the SDSS sample

      integer*4 nr__
      parameter (nr__=206)	! Number of records
      character*115 ar__   	! Full-size record

      character*6   Sample     (nr__) ! [SDSS/COSMOS] Name of sample
      character*19  Name       (nr__) ! Name (SDSS for table1 or COSMOS for table3
*                                 JHHMMSS.ss+DDMMSS.s)
      real*4        z          (nr__) ! Redshift (spectroscopic)
      real*4        umag       (nr__) ! (mag) SDSS u band AB magnitude
      real*4        gmag       (nr__) ! (mag) SDSS g band AB magnitude
      real*4        rmag       (nr__) ! (mag) SDSS r band AB magnitude
      real*4        imag       (nr__) ! (mag) SDSS i band AB magnitude
      real*4        zmag       (nr__) ! (mag) SDSS z band AB magnitude
      character*1   l_F24um    (nr__) ! Upper limit flag on F24um
      real*4        F24um      (nr__) ! (fW/m2) Spitzer/MIPS 24 micron band flux (1)
      real*4        FNUV       (nr__) ! (fW/m2) GALEX NUV band flux (1)
      real*4        E_FNUV     (nr__) ! (fW/m2) ? Upper 1{sigma} bound on FNUV (1)
      real*4        e_FNUV_1   (nr__) ! (fW/m2) ? Lower 1{sigma} bound on FNUV (1)
      real*4        FFUV       (nr__) ! (fW/m2) GALEX FUV band flux (1)
      real*4        E_FFUV     (nr__) ! (fW/m2) ? Upper 1{sigma} bound on FFUV (1)
      real*4        e_FFUV_1   (nr__) ! (fW/m2) ? Lower 1{sigma} bound on FFUV (1)
      real*4        Lbol       (nr__) ! ([10-7W]) Log of the bolometric luminosity
*Note (1): fluxes are expressed in 10^-12^erg/cm^2^/s = 10^-15^W/m^2^

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

C  Declarations for 'table3.dat'	! Observed properties of sources in the COSMOS sample

      integer*4 nr__1
      parameter (nr__1=14)	! Number of records
      character*115 ar__1  	! Full-size record

      character*6   Sample_1   (nr__1) ! [SDSS/COSMOS] Name of sample
      character*19  Name_1     (nr__1) ! Name (SDSS for table1 or COSMOS for table3
*                                 JHHMMSS.ss+DDMMSS.s)
      real*4        z_1        (nr__1) ! Redshift (spectroscopic)
      real*4        umag_1     (nr__1) ! (mag) SDSS u band AB magnitude
      real*4        gmag_1     (nr__1) ! (mag) SDSS g band AB magnitude
      real*4        rmag_1     (nr__1) ! (mag) SDSS r band AB magnitude
      real*4        imag_1     (nr__1) ! (mag) SDSS i band AB magnitude
      real*4        zmag_1     (nr__1) ! (mag) SDSS z band AB magnitude
      character*1   l_F24um_1  (nr__1) ! Upper limit flag on F24um
      real*4        F24um_1    (nr__1) ! (fW/m2) Spitzer/MIPS 24 micron band flux (1)
      real*4        FNUV_1     (nr__1) ! (fW/m2) GALEX NUV band flux (1)
      real*4        E_FNUV_2   (nr__1) ! (fW/m2) ? Upper 1{sigma} bound on FNUV (1)
      real*4        e_FNUV_3   (nr__1) ! (fW/m2) ? Lower 1{sigma} bound on FNUV (1)
      real*4        FFUV_1     (nr__1) ! (fW/m2) GALEX FUV band flux (1)
      real*4        E_FFUV_2   (nr__1) ! (fW/m2) ? Upper 1{sigma} bound on FFUV (1)
      real*4        e_FFUV_3   (nr__1) ! (fW/m2) ? Lower 1{sigma} bound on FFUV (1)
      real*4        Lbol_1     (nr__1) ! ([10-7W]) Log of the bolometric luminosity
*Note (1): fluxes are expressed in 10^-12^erg/cm^2^/s = 10^-15^W/m^2^

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

C  Loading file 'table1.dat'	! Observed properties of sources in the SDSS sample

C  Format for file interpretation

    1 format(
     +  A6,1X,A19,1X,F5.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,
     +  A1,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,
     +  F4.1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,206
        read(1,'(A115)')ar__
        read(ar__,1)
     +  Sample(i__),Name(i__),z(i__),umag(i__),gmag(i__),rmag(i__),
     +  imag(i__),zmag(i__),l_F24um(i__),F24um(i__),FNUV(i__),
     +  E_FNUV(i__),e_FNUV_1(i__),FFUV(i__),E_FFUV(i__),e_FFUV_1(i__),
     +  Lbol(i__)
        if(ar__(82:86) .EQ. '') E_FNUV(i__) = rNULL__
        if(ar__(88:92) .EQ. '') e_FNUV_1(i__) = rNULL__
        if(ar__(100:104) .EQ. '') E_FFUV(i__) = rNULL__
        if(ar__(106:110) .EQ. '') e_FFUV_1(i__) = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  Sample(i__),Name(i__),z(i__),umag(i__),gmag(i__),rmag(i__),
     +  imag(i__),zmag(i__),l_F24um(i__),F24um(i__),FNUV(i__),
     +  E_FNUV(i__),e_FNUV_1(i__),FFUV(i__),E_FFUV(i__),e_FFUV_1(i__),
     +  Lbol(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table3.dat'	! Observed properties of sources in the COSMOS sample

C  Format for file interpretation

    2 format(
     +  A6,1X,A19,1X,F5.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,
     +  A1,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,
     +  F4.1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,14
        read(1,'(A115)')ar__1
        read(ar__1,2)
     +  Sample_1(i__),Name_1(i__),z_1(i__),umag_1(i__),gmag_1(i__),
     +  rmag_1(i__),imag_1(i__),zmag_1(i__),l_F24um_1(i__),
     +  F24um_1(i__),FNUV_1(i__),E_FNUV_2(i__),e_FNUV_3(i__),
     +  FFUV_1(i__),E_FFUV_2(i__),e_FFUV_3(i__),Lbol_1(i__)
        if(ar__1(82:86) .EQ. '') E_FNUV_2(i__) = rNULL__
        if(ar__1(88:92) .EQ. '') e_FNUV_3(i__) = rNULL__
        if(ar__1(100:104) .EQ. '') E_FFUV_2(i__) = rNULL__
        if(ar__1(106:110) .EQ. '') e_FFUV_3(i__) = rNULL__
c    ..............Just test output...........
        write(6,2)
     +  Sample_1(i__),Name_1(i__),z_1(i__),umag_1(i__),gmag_1(i__),
     +  rmag_1(i__),imag_1(i__),zmag_1(i__),l_F24um_1(i__),
     +  F24um_1(i__),FNUV_1(i__),E_FNUV_2(i__),e_FNUV_3(i__),
     +  FFUV_1(i__),E_FFUV_2(i__),e_FFUV_3(i__),Lbol_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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