FORTRAN Generation
(/./ftp/cats/J/A_A/488/867)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/488/867 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/A+A/488/867       Synchrotron peak frequency of 135 AGN      (Nieppola+, 2008)
*================================================================================
*Blazar sequence - an artefact of Doppler boosting.
*    Nieppola E., Valtaoja E., Tornikoski M., Hovatta T., Kotiranta M.
*   <Astron. Astrophys., 488, 867-872 (2008)>
*   =2008A&A...488..867N
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! The sample and the observational synchrotron
                              peak frequencies obtained in this work

      integer*4 nr__
      parameter (nr__=135)	! Number of records
      character*70 ar__   	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg      (nr__) ! (deg) Right Ascension J2000
      real*8        DEdeg      (nr__) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*9   Name       (nr__) ! Source Name (HHMM+DDd or HHMM+DDMM)
      character*12  OName      (nr__) ! Other name
      integer*4     RAh        (nr__) ! (h) Right ascension (J2000)
      integer*4     RAm        (nr__) ! (min) Right ascension (J2000)
      real*4        RAs        (nr__) ! (s) Right ascension (J2000)
      character*1   DE_        (nr__) ! Declination sign (J2000)
      integer*4     DEd        (nr__) ! (deg) Declination (J2000)
      integer*4     DEm        (nr__) ! (arcmin) Declination (J2000)
      real*4        DEs        (nr__) ! (arcsec) Declination (J2000)
      character*1   Jy         (nr__) ! [*] * when in 1.2Jy AGN sample
      character*3   Class      (nr__) ! AGN Classification (3)
      real*4        lognup     (nr__) ! ([Hz]) ? Observational synchrotron peak frequency (1)
      character*1   n_lognup   (nr__) ! [1] Determination from highest flux density (2)
      real*4        z          (nr__) ! ? Redshift
      character*1   Bl         (nr__) ! [*] * when in Blazar sample
*Note (1): The values of {nu}_p_ listed here have been determined directly
*     from the SEDs and are not corrected for redshift nor for Doppler boosting.
*Note (2): 1 means that log{nu}_p_ was determined from the highest flux
*     density measurement of the synchrotron component of the SED (see Sect.3.1)
*Note (3): Classes are as follows:
*     HPQ = highly polarized quasars (>=3%)
*     LPQ = low polarization quasars (>=3%)
*     QSO = non-polarized quasars
*     BLO = BL Lac objects
*     GAM = radio galaxies

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

C  Loading file 'table1.dat'	! The sample and the observational synchrotron
*                              peak frequencies obtained in this work

C  Format for file interpretation

    1 format(
     +  A9,1X,A12,1X,I2,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F5.2,1X,A1,1X,
     +  A3,1X,F5.2,1X,A1,2X,F5.3,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,135
        read(1,'(A70)')ar__
        read(ar__,1)
     +  Name(i__),OName(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Jy(i__),Class(i__),lognup(i__),
     +  n_lognup(i__),z(i__),Bl(i__)
        if(ar__(55:59) .EQ. '') lognup(i__) = rNULL__
        if(ar__(64:68) .EQ. '') z(i__) = rNULL__
        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)
     +  Name(i__),OName(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Jy(i__),Class(i__),lognup(i__),
     +  n_lognup(i__),z(i__),Bl(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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