FORTRAN Generation
(/./ftp/cats/J/MNRAS/401/294)

Conversion of standardized ReadMe file for file /./ftp/cats/J/MNRAS/401/294 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/401/294    Optical identification of XMM-LSS sources    (Stalin+, 2010)
*================================================================================
*Optical identification of XMM sources in the Canada-France-Hawaii telescope
*legacy survey.
*    Stalin C.S., Petitjean P., Srianand R., Fox A.J., Coppolani F., Schwope A.
*   <Mon. Not. R. Astron. Soc., 401, 294-306 (2010)>
*   =2010MNRAS.401..294S
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table2.dat'	! Properties of the optical identification of the
                              XMM sources

      integer*4 nr__
      parameter (nr__=487)	! Number of records
      character*80 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)

      character*16  XLSS        ! XLSS designation (JHHMMSS.s+DDMMSS)
      integer*4     RAh         ! (h) Optical right ascension (J2000)
      integer*4     RAm         ! (min) Optical right ascension (J2000)
      real*4        RAs         ! (s) Optical right ascension (J2000)
      character*1   DE_         ! Optical declination sign (J2000)
      integer*4     DEd         ! (deg) Optical declination (J2000)
      integer*4     DEm         ! (arcmin) Optical declination (J2000)
      real*4        DEs         ! (arcsec) Optical declination (J2000)
      real*4        Sep         ! (arcsec) Angular separation between the XMM and
*                                   optical position
      real*4        g_mag       ! (mag) SDSS g' magnitude
      real*4        z           ! Spectroscopic redshift
      integer*4     q_z         ! [1/3] Quality of redshift (1=secure)i (3)
      real*4        alpha       ! Broad-band spectral index (1)
      character*3   Class       ! This paper spectroscopic identification (2)
      character*5   Inst        ! [SWIRE ] SWIRE for objects detected by Spitzer
*Note (1): Broad-band spectral index,
*          alpha_ox_=[log(L_X_/L_opt_)]/[log(nu_X_/nu_opt_)]
*Note (2): Classes are:
*    ALG = Absorption-line galaxy (at z<0.76)
*    ELG = Emission-Line galaxy (at z<0.76)
*    QSO = Quasar or broad-line AGN
*    STA = Galactic stellar source
*Note (3): Quality of the redshift is:
*      1 = secure (two or more lines identified in the spectrum)
*      2 = only 1 broad/narrow emission/absorption line (ambiguous redshift)
*      3 = spectrum of poor quality

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

C  Loading file 'table2.dat'	! Properties of the optical identification of the
*                              XMM sources

C  Format for file interpretation

    1 format(
     +  5X,A16,1X,I1,1X,I2,1X,F6.3,1X,A1,I1,1X,I2,1X,F6.3,1X,F4.2,1X,
     +  F5.2,1X,F4.2,1X,I1,1X,F5.2,1X,A3,1X,A5)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,487
        read(1,'(A80)')ar__
        read(ar__,1)
     +  XLSS,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Sep,g_mag,z,q_z,alpha,Class,
     +  Inst
        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)
     +  XLSS,RAh,RAm,RAs,DE_,DEd,DEm,DEs,Sep,g_mag,z,q_z,alpha,Class,
     +  Inst
        write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c    .......End.of.Just test output...........
      end do
      close(1)

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