FORTRAN Generation
(/./ftp/cats/J/AJ/138/1116)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AJ/138/1116 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_1.8, on 2014-Sep-16
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__=-1.e37)     	! NULL real number
      parameter  (iNULL__=-2147483647)	! NULL int  number

C=============================================================================
Cat. J/AJ/138/1116            A Spitzer view of NGC 2264                (Sung+, 2009)
*================================================================================
*A Spitzer view of the young open cluster NGC 2264.
*    Sung H., Stauffer J.R., Bessell M.S.
*   <Astron. J., 138, 1116-1136 (2009)>
*   =2009AJ....138.1116S
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Catalog of sources detected with Spitzer Space
                             Telescope IRAC and MIPS 24 micron

      integer*4 nr__
      parameter (nr__=21991)	! Number of records
      character*165 ar__   	! Full-size record

      real*8        RA_        (nr__) ! (deg) Right Ascension J2000
      real*8        Dec        (nr__) ! (deg)     Declination J2000
      integer*4     SST        (nr__) ! Running identification number (G1)
      integer*4     RAh        (nr__) ! (h) Hour of Right Ascension (J2000)
      integer*4     RAm        (nr__) ! (min) Minute of Right Ascension (J2000)
      real*4        RAs        (nr__) ! (s) Second of Right Ascension (J2000)
      character*1   DE_        (nr__) ! Sign of Declination (J2000)
      integer*4     DEd        (nr__) ! (deg) Degree of Declination (J2000)
      integer*4     DEm        (nr__) ! (arcmin) Arcminute of Declination (J2000)
      real*4        DEs        (nr__) ! (arcsec) Arcsecond of Declination (J2000)
      real*4        v_3_6_     (nr__) ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude
      real*4        v_4_5_     (nr__) ! (mag) ? Spitzer/IRAC 4.5 micron band magnitude
      real*4        v_5_8_     (nr__) ! (mag) ? Spitzer/IRAC 5.8 micron band magnitude
      real*4        v_8_0_     (nr__) ! (mag) ? Spitzer/IRAC 8.0 micron band magnitude
      real*4        v_24_      (nr__) ! (mag) ? Spitzer/MIPS 24 micron band magnitude
      real*4        e__3_6_    (nr__) ! (mag) ? Uncertainty in [3.6]
      real*4        e__4_5_    (nr__) ! (mag) ? Uncertainty in [4.5]
      real*4        e__5_8_    (nr__) ! (mag) ? Uncertainty in [5.8]
      real*4        e__8_0_    (nr__) ! (mag) ? Uncertainty in [8.0]
      real*4        e__24_     (nr__) ! (mag) ? Uncertainty in [24]
      integer*4     o__3_6_    (nr__) ! Number of [3.6] observations
      integer*4     o__4_5_    (nr__) ! Number of [4.5] observations
      integer*4     o__5_8_    (nr__) ! Number of [5.8] observations
      integer*4     o__8_0_    (nr__) ! Number of [8.0] observations
      integer*4     o__24_     (nr__) ! Number of [24] observations
      character*1   Dup        (nr__) ! [D/T] Duplicity code (1)
      character*8   Mem        (nr__) ! Membership (2)
      character*16  v2MASS     (nr__) ! 2MASS identification (HHMMSSss+DDMMSSs)
      character*20  Sung       (nr__) ! Sung et al. identification(s) (G2)
      character*13  Note       (nr__) ! Counterparts of weak X-ray source (3)
*Note (1):  Code as follows:
*    D = SST source having two optical counterparts within 2" searching radii;
*    T = SST source having three optical counterparts within 2" searching radii.
*Note (2): IR classification (Class I, II, II/III, pre-TD (pre-transition disk),
*          and TD(transition disk)) and other membership listed in
*          Sung et al. (2008, Cat. J/AJ/135/441) as follows:
*  H = H{alpha} emission star,
*  h = H{alpha} emission candidate;
*  X = X-ray emission star,
*  x = X-ray emission candidate;
*  + = H{alpha} emission star with X-ray emission,
*  - = H{alpha} emission candidate with X-ray emission,
*  E = strong H{alpha} emission star from spectroscopy (EWHa>=10{AA} in Dahm &
*      Simon (2005, Cat. J/AJ/129/829) or H{alpha} index >=2.5 in Reipurth et al.
*      (2004, Cat. J/AJ/127/1117)),
*  e = weak H{alpha} emission star from spectroscopy (EWHa<10{AA} in Dahm & Simon
*      (2005, Cat. J/AJ/129/829) or H{alpha} index <=2 in Reipurth et al. (2004,
*      Cat. J/AJ/127/1117));
*  M = X-ray emission star with membership class "e", i.e. "M"="e"+"X".
*  P = X-ray emission star with membership class "E", i.e. "P"="E"+"X";
*  p = X-ray candidate with membership class "E", i.e. "p"="E"+"x".
*Note (3): 30 IRAC sources as counterparts of weak X-ray sources with
*          significance between 3.3 and 5.0.

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

C  Declarations for 'table2.dat'	! Spitzer counterparts of X-ray sources without
                             optical or 2MASS counterparts

      integer*4 nr__1
      parameter (nr__1=43)	! Number of records
      character*117 ar__1  	! Full-size record

      real*8        RA__1      (nr__1) ! (deg) Right Ascension J2000
      real*8        Dec_1      (nr__1) ! (deg)     Declination J2000
      integer*4     SST_1      (nr__1) ! Running identification number (G1)
      integer*4     RAh_1      (nr__1) ! (h) Hour of Right Ascension (J2000)
      integer*4     RAm_1      (nr__1) ! (min) Minute of Right Ascension (J2000)
      real*4        RAs_1      (nr__1) ! (s) Second of Right Ascension (J2000)
      character*1   DE__1      (nr__1) ! Sign of declination (J2000)
      integer*4     DEd_1      (nr__1) ! (deg) Degree of Declination (J2000)
      integer*4     DEm_1      (nr__1) ! (arcmin) Arcminute of Declination (J2000)
      real*4        DEs_1      (nr__1) ! (arcsec) Arcsecond of Declination (J2000)
      real*4        v_3_6__1   (nr__1) ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude
      real*4        v_4_5__1   (nr__1) ! (mag) Spitzer/IRAC 4.5 micron band magnitude
      real*4        v_5_8__1   (nr__1) ! (mag) ? Spitzer/IRAC 5.8 micron band magnitude
      real*4        v_8_0__1   (nr__1) ! (mag) ? Spitzer/IRAC 8.0 micron band magnitude
      real*4        v_24__1    (nr__1) ! (mag) ? Spitzer/MIPS 24 micron band magnitude
      real*4        e__3_6__1  (nr__1) ! (mag) ? Uncertainty in [3.6]
      real*4        e__4_5__1  (nr__1) ! (mag) Uncertainty in [4.5]
      real*4        e__5_8__1  (nr__1) ! (mag) ? Uncertainty in [5.8]
      real*4        e__8_0__1  (nr__1) ! (mag) ? Uncertainty in [8.0]
      real*4        e__24__1   (nr__1) ! (mag) ? Uncertainty in [24]
      integer*4     o__3_6__1  (nr__1) ! Number of [3.6] observations
      integer*4     o__4_5__1  (nr__1) ! Number of [4.5] observations
      integer*4     o__5_8__1  (nr__1) ! Number of [5.8] observations
      integer*4     o__8_0__1  (nr__1) ! Number of [8.0] observations
      integer*4     o__24__1   (nr__1) ! Number of [24] observations
      character*6   Class      (nr__1) ! Object classification (Galaxy, I, II or II/III)
      real*4        Signi      (nr__1) ! X-ray detection significance (1)
      real*4        Dist       (nr__1) ! (arcsec) Distance Spitzer/X-ray
*Note (1): X-ray detection significance from "pwdetect" (see Sung et al. 2004,
*          Cat. J/AJ/128/1684; Flaccomio et al. 2006, Cat. J/A+A/455/903).

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

C  Declarations for 'table3.dat'	! Variables detected in IRAC [3.6] and [4.5]

      integer*4 nr__2
      parameter (nr__2=28)	! Number of records
      character*102 ar__2  	! Full-size record

      integer*4     SST_2      (nr__2) ! Running identification number (G1)
      character*1   f_SST      (nr__2) ! [a] long exposure images used (1)
      real*4        v_3_6_6    (nr__2) ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude on
*                                  2004 Mar 6
      real*4        e__3_6_6   (nr__2) ! (mag) ? Uncertainty in [3.6]
      real*4        v_3_6_8    (nr__2) ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude on
*                                  2004 Oct 8
      real*4        e__3_6_8   (nr__2) ! (mag) ? Uncertainty in [3.6]
      real*4        d_3_6_     (nr__2) ! (mag) ? [3.6] difference
      real*4        v_4_5_6    (nr__2) ! (mag) ? Spitzer/IRAC [4.5 micron band magnitude on
*                                  2004 Mar 6
      real*4        e__4_5_6   (nr__2) ! (mag) ? Uncertainty in [4.5]
      real*4        v_4_5_8    (nr__2) ! (mag) ? Spitzer/IRAC 4.5 micron band magnitude on
*                                  2004 Oct 8
      real*4        e__4_5_8   (nr__2) ! (mag) ? Uncertainty in [4.5]
      real*4        d_4_5_     (nr__2) ! (mag) ? [4.5] difference
      character*6   Class_1    (nr__2) ! Infra-red classification (I, II or II/III)
      character*8   Other      (nr__2) ! Other classification (X or X+Halpha)
      character*13  OName      (nr__2) ! Sung et al. identification(s) (G2)
*Note (1):
*  a = Used only data from long exposure images because short and long exposure
*     images show large systematic differences probably due to the nearby
*     bright star SST 13808.

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

C  Declarations for 'table5.dat'	! New BMS star candidates (stars below the
                             pre-main-sequence locus)

      integer*4 nr__3
      parameter (nr__3=10)	! Number of records
      character*82 ar__3  	! Full-size record

      integer*4     SST_3      (nr__3) ! Running identification number (G1)
      character*1   n_SST      (nr__3) ! [bc] Note on source (1)
      character*13  OName_1    (nr__3) ! Sung et al. identification(s) (G2)
      real*4        v_3_6__2   (nr__3) ! (mag) Spitzer/IRAC 3.6 micron band magnitude
      real*4        v_4_5__2   (nr__3) ! (mag) Spitzer/IRAC 4.5 micron band magnitude
      real*4        v_5_8__2   (nr__3) ! (mag) Spitzer/IRAC 5.8 micron band magnitude
      real*4        v_8_0__2   (nr__3) ! (mag) Spitzer/IRAC 8.0 micron band magnitude
      real*4        v_24__2    (nr__3) ! (mag) ? Spitzer/MIPS 24 micron band magnitude
      character*3   Ha_        (nr__3) ! [Yes/No/? ] H{alpha} emission?
      character*2   Class_2    (nr__3) ! IR classification (I or II)
      real*4        SED        (nr__3) ! SED slope
      real*4        e_SED      (nr__3) ! SED uncertainty
      real*4        Qcc        (nr__3) ! Mean value of a YSO class Q_CC_ (2)
      real*4        D_I        (nr__3) ! Magnitude difference from the faint limit of
*                                 the PMS locus in NGC 2264
*Note (1): Flag as follows:
*  b = If the actual optical counterpart of SST 10184 is C30962, then SST 10184
*      may be a SFG with PAH emission. See Section 2.5.
*  c = Ogura (1984PASJ...36..139O) noted as an H{alpha} emission star, but no
*      signature of H{alpha} emission from CCD photometry was detected.
*Note (2): The mean value of a YSO class (Cl_i_) (call this quantity Q_CC_) is:
*          Q_CC_={Sigma}_i_Cl_i_xq_i_xw_i_/{Sigma}_i_q_i_xw_i_
*          where q_i_ and w_i_ are different weights. See section 3.1.

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

C  Loading file 'table1.dat'	! Catalog of sources detected with Spitzer Space
*                             Telescope IRAC and MIPS 24 micron

C  Format for file interpretation

    1 format(
     +  I5,1X,I1,1X,I2,1X,F5.2,1X,A1,I2,1X,I2,1X,F4.1,1X,F6.3,1X,F6.3,
     +  1X,F6.3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,
     +  F5.3,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,A1,1X,A8,1X,A16,1X,A20,
     +  1X,A13)

C  Effective file loading

      open(unit=1,file='table1.dat', status='old')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,21991
        read(1,'(A165)')ar__
        read(ar__,1)
     +  SST(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
     +  DEm(i__),DEs(i__),v_3_6_(i__),v_4_5_(i__),v_5_8_(i__),
     +  v_8_0_(i__),v_24_(i__),e__3_6_(i__),e__4_5_(i__),e__5_8_(i__),
     +  e__8_0_(i__),e__24_(i__),o__3_6_(i__),o__4_5_(i__),
     +  o__5_8_(i__),o__8_0_(i__),o__24_(i__),Dup(i__),Mem(i__),
     +  v2MASS(i__),Sung(i__),Note(i__)
        if(ar__(30:35) .EQ. '') v_3_6_(i__) = rNULL__
        if(ar__(37:42) .EQ. '') v_4_5_(i__) = rNULL__
        if(ar__(44:49) .EQ. '') v_5_8_(i__) = rNULL__
        if(ar__(51:56) .EQ. '') v_8_0_(i__) = rNULL__
        if(ar__(58:62) .EQ. '') v_24_(i__) = rNULL__
        if(ar__(64:68) .EQ. '') e__3_6_(i__) = rNULL__
        if(ar__(70:74) .EQ. '') e__4_5_(i__) = rNULL__
        if(ar__(76:80) .EQ. '') e__5_8_(i__) = rNULL__
        if(ar__(82:86) .EQ. '') e__8_0_(i__) = rNULL__
        if(ar__(88:92) .EQ. '') e__24_(i__) = rNULL__
c       Derive coordinates RA_ and Dec from input data
c       (RA_ and Dec are set to rNULL_ when unknown)
        RA_(i__) = RAh(i__)
        if(RAh(i__) .GE. 0) RA_(i__)=RAh(i__)*15.
        if(RAm(i__) .GE. 0) RA_(i__)=RA_(i__)+RAm(i__)/4.
        if(RAs(i__) .GE. 0) RA_(i__)=RA_(i__)+RAs(i__)/240.
        Dec(i__) = DEd(i__)
        if(DEm(i__) .GE. 0) Dec(i__)=Dec(i__)+DEm(i__)/60.
        if(DEs(i__) .GE. 0) Dec(i__)=Dec(i__)+DEs(i__)/3600.
        if(DE_(i__).EQ.'-'.AND.Dec(i__).GE.0) Dec(i__)=-Dec(i__)
c    ..............Just test output...........
        write(6,1)
     +  SST(i__),RAh(i__),RAm(i__),RAs(i__),DE_(i__),DEd(i__),
     +  DEm(i__),DEs(i__),v_3_6_(i__),v_4_5_(i__),v_5_8_(i__),
     +  v_8_0_(i__),v_24_(i__),e__3_6_(i__),e__4_5_(i__),e__5_8_(i__),
     +  e__8_0_(i__),e__24_(i__),o__3_6_(i__),o__4_5_(i__),
     +  o__5_8_(i__),o__8_0_(i__),o__24_(i__),Dup(i__),Mem(i__),
     +  v2MASS(i__),Sung(i__),Note(i__)
        write(6,'(6H Pos: 2F8.4)') RA_(i__),Dec(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table2.dat'	! Spitzer counterparts of X-ray sources without
*                             optical or 2MASS counterparts

C  Format for file interpretation

    2 format(
     +  I5,1X,I1,1X,I2,1X,F5.2,1X,A1,I1,1X,I2,1X,F4.1,1X,F6.3,1X,F6.3,
     +  1X,F6.3,1X,F6.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,F5.3,1X,
     +  F5.3,1X,I1,1X,I1,1X,I1,1X,I1,1X,I1,1X,A6,1X,F4.1,1X,F3.1)

C  Effective file loading

      open(unit=1,file='table2.dat', status='old')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,43
        read(1,'(A117)')ar__1
        read(ar__1,2)
     +  SST_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
     +  DEd_1(i__),DEm_1(i__),DEs_1(i__),v_3_6__1(i__),v_4_5__1(i__),
     +  v_5_8__1(i__),v_8_0__1(i__),v_24__1(i__),e__3_6__1(i__),
     +  e__4_5__1(i__),e__5_8__1(i__),e__8_0__1(i__),e__24__1(i__),
     +  o__3_6__1(i__),o__4_5__1(i__),o__5_8__1(i__),o__8_0__1(i__),
     +  o__24__1(i__),Class(i__),Signi(i__),Dist(i__)
        if(ar__1(29:34) .EQ. '') v_3_6__1(i__) = rNULL__
        if(ar__1(43:48) .EQ. '') v_5_8__1(i__) = rNULL__
        if(ar__1(50:55) .EQ. '') v_8_0__1(i__) = rNULL__
        if(ar__1(57:61) .EQ. '') v_24__1(i__) = rNULL__
        if(ar__1(63:67) .EQ. '') e__3_6__1(i__) = rNULL__
        if(ar__1(75:79) .EQ. '') e__5_8__1(i__) = rNULL__
        if(ar__1(81:85) .EQ. '') e__8_0__1(i__) = rNULL__
        if(ar__1(87:91) .EQ. '') e__24__1(i__) = rNULL__
c       Derive coordinates RA__1 and Dec_1 from input data
c       (RA__1 and Dec_1 are set to rNULL_ when unknown)
        RA__1(i__) = RAh_1(i__)
        if(RAh_1(i__) .GE. 0) RA__1(i__)=RAh_1(i__)*15.
        if(RAm_1(i__) .GE. 0) RA__1(i__)=RA__1(i__)+RAm_1(i__)/4.
        if(RAs_1(i__) .GE. 0) RA__1(i__)=RA__1(i__)+RAs_1(i__)/240.
        Dec_1(i__) = DEd_1(i__)
        if(DEm_1(i__) .GE. 0) Dec_1(i__)=Dec_1(i__)+DEm_1(i__)/60.
        if(DEs_1(i__) .GE. 0) Dec_1(i__)=Dec_1(i__)+DEs_1(i__)/3600.
        if(DE__1(i__).EQ.'-'.AND.Dec_1(i__).GE.0) Dec_1(i__)=-Dec_1(i__)
c    ..............Just test output...........
        write(6,2)
     +  SST_1(i__),RAh_1(i__),RAm_1(i__),RAs_1(i__),DE__1(i__),
     +  DEd_1(i__),DEm_1(i__),DEs_1(i__),v_3_6__1(i__),v_4_5__1(i__),
     +  v_5_8__1(i__),v_8_0__1(i__),v_24__1(i__),e__3_6__1(i__),
     +  e__4_5__1(i__),e__5_8__1(i__),e__8_0__1(i__),e__24__1(i__),
     +  o__3_6__1(i__),o__4_5__1(i__),o__5_8__1(i__),o__8_0__1(i__),
     +  o__24__1(i__),Class(i__),Signi(i__),Dist(i__)
        write(6,'(6H Pos: 2F8.4)') RA__1(i__),Dec_1(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table3.dat'	! Variables detected in IRAC [3.6] and [4.5]

C  Format for file interpretation

    3 format(
     +  I5,A1,1X,F6.3,1X,F5.3,1X,F6.3,1X,F5.3,1X,F6.3,1X,F6.3,1X,F5.3,
     +  1X,F6.3,1X,F5.3,1X,F6.3,1X,A6,1X,A8,1X,A13)

C  Effective file loading

      open(unit=1,file='table3.dat', status='old')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,28
        read(1,'(A102)')ar__2
        read(ar__2,3)
     +  SST_2(i__),f_SST(i__),v_3_6_6(i__),e__3_6_6(i__),v_3_6_8(i__),
     +  e__3_6_8(i__),d_3_6_(i__),v_4_5_6(i__),e__4_5_6(i__),
     +  v_4_5_8(i__),e__4_5_8(i__),d_4_5_(i__),Class_1(i__),
     +  Other(i__),OName(i__)
        if(ar__2(8:13) .EQ. '') v_3_6_6(i__) = rNULL__
        if(ar__2(15:19) .EQ. '') e__3_6_6(i__) = rNULL__
        if(ar__2(21:26) .EQ. '') v_3_6_8(i__) = rNULL__
        if(ar__2(28:32) .EQ. '') e__3_6_8(i__) = rNULL__
        if(ar__2(34:39) .EQ. '') d_3_6_(i__) = rNULL__
        if(ar__2(41:46) .EQ. '') v_4_5_6(i__) = rNULL__
        if(ar__2(48:52) .EQ. '') e__4_5_6(i__) = rNULL__
        if(ar__2(54:59) .EQ. '') v_4_5_8(i__) = rNULL__
        if(ar__2(61:65) .EQ. '') e__4_5_8(i__) = rNULL__
        if(ar__2(67:72) .EQ. '') d_4_5_(i__) = rNULL__
c    ..............Just test output...........
        write(6,3)
     +  SST_2(i__),f_SST(i__),v_3_6_6(i__),e__3_6_6(i__),v_3_6_8(i__),
     +  e__3_6_8(i__),d_3_6_(i__),v_4_5_6(i__),e__4_5_6(i__),
     +  v_4_5_8(i__),e__4_5_8(i__),d_4_5_(i__),Class_1(i__),
     +  Other(i__),OName(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table5.dat'	! New BMS star candidates (stars below the
*                             pre-main-sequence locus)

C  Format for file interpretation

    4 format(
     +  I5,A1,1X,A13,1X,F6.3,1X,F6.3,1X,F6.3,1X,F6.3,1X,F5.3,1X,A3,1X,
     +  A2,1X,F5.2,1X,F4.2,1X,F3.1,1X,F5.2)

C  Effective file loading

      open(unit=1,file='table5.dat', status='old')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,10
        read(1,'(A82)')ar__3
        read(ar__3,4)
     +  SST_3(i__),n_SST(i__),OName_1(i__),v_3_6__2(i__),
     +  v_4_5__2(i__),v_5_8__2(i__),v_8_0__2(i__),v_24__2(i__),
     +  Ha_(i__),Class_2(i__),SED(i__),e_SED(i__),Qcc(i__),D_I(i__)
        if(ar__3(50:54) .EQ. '') v_24__2(i__) = rNULL__
c    ..............Just test output...........
        write(6,4)
     +  SST_3(i__),n_SST(i__),OName_1(i__),v_3_6__2(i__),
     +  v_4_5__2(i__),v_5_8__2(i__),v_8_0__2(i__),v_24__2(i__),
     +  Ha_(i__),Class_2(i__),SED(i__),e_SED(i__),Qcc(i__),D_I(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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