FORTRAN Generation
(/./ftp/cats/J/AZh/77/619)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AZh/77/619 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-29
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/AZh/77/619    Energy distributions in giants and supergiants (Knyazeva+, 2000)
*================================================================================
*The normal energy distributions in stellar spectra: giants and supergiants.
*    Knyazeva L.N., Kharitonov A.V.
*   <Astron. Zh. 77, 619 (2000)>
*   =2000AZh....77..619K
*   =2000ARep...44..548K
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Giants used to derive the normal energy distributions

      integer*4 nr__
      parameter (nr__=56)	! Number of records
      character*72 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*5   SpType     (nr__) ! MK Spectral type
      character*9   Name       (nr__) ! Name of the star
      character*1   n_Name     (nr__) ! [*] *: star is considered as unreddened
      integer*4     RAh        (nr__) ! (h) Right ascension (J2000)
      integer*4     RAm        (nr__) ! (min) Right ascension (J2000)
      real*8        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)
      real*4        Vmag       (nr__) ! (mag) V magnitude
      real*4        B_V        (nr__) ! (mag) B-V color index
      real*4        Plx        (nr__) ! (arcsec) ? Trigonometric parallax
      integer*4     GLAT       (nr__) ! (deg) Galactic latitude
      character*5   Ref        (nr__) ! References to spectrophotometric data (G1)

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

C  Declarations for 'table2.dat'	! Supergiants used to derive the normal energy
                           distributions

      integer*4 nr__1
      parameter (nr__1=22)	! Number of records
      character*78 ar__1  	! Full-size record

C  J2000 position composed of: RAh RAm RAs DE- DEd DEm DEs
      real*8        RAdeg_1    (nr__1) ! (deg) Right Ascension J2000
      real*8        DEdeg_1    (nr__1) ! (deg)     Declination J2000
C  ---------------------------------- ! (position vector(s) in degrees)

      character*7   SpType_1   (nr__1) ! MK Spectral type
      character*9   Name_1     (nr__1) ! Name of the star
      character*1   n_Name_1   (nr__1) ! [*] *: star is considered as unreddened
      integer*4     RAh_1      (nr__1) ! (h) Right ascension (J2000)
      integer*4     RAm_1      (nr__1) ! (min) Right ascension (J2000)
      real*8        RAs_1      (nr__1) ! (s) Right ascension (J2000)
      character*1   DE__1      (nr__1) ! Declination sign (J2000)
      integer*4     DEd_1      (nr__1) ! (deg) Declination (J2000)
      integer*4     DEm_1      (nr__1) ! (arcmin) Declination (J2000)
      real*4        DEs_1      (nr__1) ! (arcsec) Declination (J2000)
      real*4        Vmag_1     (nr__1) ! (mag) V magnitude
      real*4        B_V_1      (nr__1) ! (mag) B-V color index
      real*4        Plx_1      (nr__1) ! (arcsec) ? Trigonometric parallax
      integer*4     GLAT_1     (nr__1) ! (deg) Galactic latitude
      real*4        E_B_V      (nr__1) ! (mag) ? Color excess
      character*5   Ref_1      (nr__1) ! References to spectrophotometric data (G1)

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

C  Declarations for 'table5.dat'	! Normal color indices of stars in the WBVR
                           (Kornilov et al., 1991, Tr. Gos. Astron. Inst.
                           Shternberga 63) system

      integer*4 nr__2
      parameter (nr__2=81)	! Number of records
      character*27 ar__2  	! Full-size record

      character*8   SpType_2   (nr__2) ! MK Spectral type
      real*4        v_B_V_0    (nr__2) ! (mag) (B-V)0 color index
      real*4        v_W_B_0    (nr__2) ! (mag) (W-B)0 color index

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

C  Loading file 'table1.dat'	! Giants used to derive the normal energy distributions

C  Format for file interpretation

    1 format(
     +  A5,1X,A9,A1,1X,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F6.3,1X,
     +  F4.2,1X,F5.2,1X,F5.3,2X,I3,1X,A5)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,56
        read(1,'(A72)')ar__
        read(ar__,1)
     +  SpType(i__),Name(i__),n_Name(i__),RAh(i__),RAm(i__),RAs(i__),
     +  DE_(i__),DEd(i__),DEm(i__),DEs(i__),Vmag(i__),B_V(i__),
     +  Plx(i__),GLAT(i__),Ref(i__)
        if(ar__(57:61) .EQ. '') Plx(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)
     +  SpType(i__),Name(i__),n_Name(i__),RAh(i__),RAm(i__),RAs(i__),
     +  DE_(i__),DEd(i__),DEm(i__),DEs(i__),Vmag(i__),B_V(i__),
     +  Plx(i__),GLAT(i__),Ref(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg(i__),DEdeg(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table2.dat'	! Supergiants used to derive the normal energy
*                           distributions

C  Format for file interpretation

    2 format(
     +  A7,1X,A9,A1,I2,1X,I2,1X,F7.4,1X,A1,I2,1X,I2,1X,F6.3,1X,F4.2,
     +  1X,F5.2,1X,F5.3,1X,I3,1X,F4.2,2X,A5)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,22
        read(1,'(A78)')ar__1
        read(ar__1,2)
     +  SpType_1(i__),Name_1(i__),n_Name_1(i__),RAh_1(i__),RAm_1(i__),
     +  RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
     +  Vmag_1(i__),B_V_1(i__),Plx_1(i__),GLAT_1(i__),E_B_V(i__),
     +  Ref_1(i__)
        if(ar__1(58:62) .EQ. '') Plx_1(i__) = rNULL__
        if(ar__1(68:71) .EQ. '') E_B_V(i__) = rNULL__
        RAdeg_1(i__) = rNULL__
        DEdeg_1(i__) = rNULL__
c  Derive coordinates RAdeg_1 and DEdeg_1 from input data
c  (RAdeg_1 and DEdeg_1 are set to rNULL__ when unknown)
        if(RAh_1(i__) .GT. -180) RAdeg_1(i__)=RAh_1(i__)*15.
        if(RAm_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAm_1(i__)/4.
        if(RAs_1(i__) .GT. -180) RAdeg_1(i__)=RAdeg_1(i__)+RAs_1(i__)/240.
        if(DEd_1(i__) .GE. 0) DEdeg_1(i__)=DEd_1(i__)
        if(DEm_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEm_1(i__)/60.
        if(DEs_1(i__) .GE. 0) DEdeg_1(i__)=DEdeg_1(i__)+DEs_1(i__)/3600.
        if(DE__1(i__).EQ.'-'.AND.DEdeg_1(i__).GE.0) DEdeg_1(i__)=-DEdeg_1(i__)
c    ..............Just test output...........
        write(6,2)
     +  SpType_1(i__),Name_1(i__),n_Name_1(i__),RAh_1(i__),RAm_1(i__),
     +  RAs_1(i__),DE__1(i__),DEd_1(i__),DEm_1(i__),DEs_1(i__),
     +  Vmag_1(i__),B_V_1(i__),Plx_1(i__),GLAT_1(i__),E_B_V(i__),
     +  Ref_1(i__)
        write(6,'(6H Pos: 2F8.4)') RAdeg_1(i__),DEdeg_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table5.dat'	! Normal color indices of stars in the WBVR
*                           (Kornilov et al., 1991, Tr. Gos. Astron. Inst.
*                           Shternberga 63) system

C  Format for file interpretation

    3 format(A8,1X,F6.3,2X,F6.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table5.dat')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,81
        read(1,'(A27)')ar__2
        read(ar__2,3)SpType_2(i__),v_B_V_0(i__),v_W_B_0(i__)
c    ..............Just test output...........
        write(6,3)SpType_2(i__),v_B_V_0(i__),v_W_B_0(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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