FORTRAN Generation
(/./ftp/cats/II/223/)

Conversion of standardized ReadMe file for file /./ftp/cats/II/223/ 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 2018-Feb-26
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. II/223   First Byurakan Survey (FBS), 2nd Program (Abrahamian et al., 1990-1996)
*================================================================================
*First Byurakan Survey (FBS), 2nd Program
*     Abrahamian et al.
*    <Astrophysics 32, 14 (1990); 33, 418 (1990); 33, 493 (1990);
*     34, 7 (1991); 36, 62 (1993); 36, 306 (1993); 37, 27 (1994);
*     37, 117 (1994); 37, 224 (1994); 38, 108 (1995); 39, 315 (1996) >
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'fbs2.dat'	! The second part of the First Byurakan Survey

      integer*4 nr__
      parameter (nr__=1103)	! Number of records
      character*68 ar__   	! Full-size record

C  B1950 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg      (nr__) ! (deg) Right Ascension B1950
      real*8        DEdeg      (nr__) ! (deg)     Declination B1950
C  ---------------------------------- ! (position vector(s) in degrees)

      integer*4     Seq        (nr__) ! [1,1103]+ Sequential number (FBS B NNNN)
      character*9   FBS        (nr__) ! FBS named based on B1950 position
      integer*4     RAh        (nr__) ! (h) Right Ascension B1950 (hours)
      integer*4     RAm        (nr__) ! (min) Right Ascension B1950 (minutes)
      real*4        RAs        (nr__) ! (s) Right Ascension B1950 (seconds)
      character*1   DE_        (nr__) ! Declination B1950 (sign)
      integer*4     DEd        (nr__) ! (deg) Declination B1950 (degrees)
      integer*4     DEm        (nr__) ! (arcmin) Declination B1950 (minutes)
      integer*4     DEs        (nr__) ! (arcsec) ? Declination B1950 (seconds)
      real*4        Bmag       (nr__) ! (mag) Photographic magnitude
      character*1   aType      (nr__) ! [QG*] abbreviation for QSO, Galaxy or Star
      character*4   Type       (nr__) ! *Type of the object
      character*5   SpType     (nr__) ! Spectral type for stars
      character*3   survey     (nr__) ! *Existence in other survey
      real*4        Mag2       (nr__) ! (mag) ? Magnitude from survey
      real*4        z          (nr__) ! ? Redshift, when known
      character*8   Name       (nr__) ! Other name of the source
*Note on Type: this Type is made of two parameters:
*  1. The first parameter (related to B-V index) describes the ratio of
*     the intensities of the red and blue regions of the spectrum:
*     'B' means that the blue part is stronger than the red part
*     'N' means that the intensities of the two parts are equal
*  2. The second parameter (related to U-B index) characterizes the
*     intensity of the ultraviolet region of the spectrum:
*     '1' means that the blue-violet  part is approximately 1.5 times
*         longer than the red-yellow part
*     '3' means that the blue-violet  part is approximately as long as
*         the red-yellow part
*     '2' describes the intermediate situation.
*  In addition, the existence of emission details is noted by 'e' or 'e:',
*  and absorption details by 'a' or 'a:'
*Note on survey: the other surveys are
*   PG = Palomar Green survey (see Cat. <II/207>)
*   CBS = Case Blue Stars (Pesch and Sanduleak, 1983-95)
*   CSO = Case Stellar Objects (Pesch and Sanduleak, 1983-95)
*   KUV = Kiso UV excess objects (Nogushi et al., 1980AnTok..18...55N)

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

C  Loading file 'fbs2.dat'	! The second part of the First Byurakan Survey

C  Format for file interpretation

    1 format(
     +  I4,1X,A9,1X,I2,I2,F4.1,A1,I2,I2,I2,1X,F4.1,A1,A4,1X,A5,A3,
     +  F5.2,F5.3,1X,A8)

C  Effective file loading

      open(unit=1,status='old',file=
     +'fbs2.dat')
      write(6,*) '....Loading file: fbs2.dat'
      do i__=1,1103
        read(1,'(A68)')ar__
        read(ar__,1)
     +  Seq(i__),FBS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Bmag(i__),aType(i__),Type(i__),
     +  SpType(i__),survey(i__),Mag2(i__),z(i__),Name(i__)
        if(ar__(29:30) .EQ. '') DEs(i__) = iNULL__
        if(ar__(50:54) .EQ. '') Mag2(i__) = rNULL__
        if(ar__(55:59) .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)
     +  Seq(i__),FBS(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),
     +  DEd(i__),DEm(i__),DEs(i__),Bmag(i__),aType(i__),Type(i__),
     +  SpType(i__),survey(i__),Mag2(i__),z(i__),Name(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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