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 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-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/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

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)

      integer*4     SST         ! Running identification number (G1)
      integer*4     RAh         ! (h) Hour of Right Ascension (J2000)
      integer*4     RAm         ! (min) Minute of Right Ascension (J2000)
      real*4        RAs         ! (s) Second of Right Ascension (J2000)
      character*1   DE_         ! Sign of Declination (J2000)
      integer*4     DEd         ! (deg) Degree of Declination (J2000)
      integer*4     DEm         ! (arcmin) Arcminute of Declination (J2000)
      real*4        DEs         ! (arcsec) Arcsecond of Declination (J2000)
      real*4        v_3_6_      ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude
      real*4        v_4_5_      ! (mag) ? Spitzer/IRAC 4.5 micron band magnitude
      real*4        v_5_8_      ! (mag) ? Spitzer/IRAC 5.8 micron band magnitude
      real*4        v_8_0_      ! (mag) ? Spitzer/IRAC 8.0 micron band magnitude
      real*4        v_24_       ! (mag) ? Spitzer/MIPS 24 micron band magnitude
      real*4        e__3_6_     ! (mag) ? Uncertainty in [3.6]
      real*4        e__4_5_     ! (mag) ? Uncertainty in [4.5]
      real*4        e__5_8_     ! (mag) ? Uncertainty in [5.8]
      real*4        e__8_0_     ! (mag) ? Uncertainty in [8.0]
      real*4        e__24_      ! (mag) ? Uncertainty in [24]
      integer*4     o__3_6_     ! Number of [3.6] observations
      integer*4     o__4_5_     ! Number of [4.5] observations
      integer*4     o__5_8_     ! Number of [5.8] observations
      integer*4     o__8_0_     ! Number of [8.0] observations
      integer*4     o__24_      ! Number of [24] observations
      character*1   Dup         ! [D/T] Duplicity code (1)
      character*8   Mem         ! Membership (2)
      character*16  v2MASS      ! 2MASS identification (HHMMSSss+DDMMSSs)
      character*20  Sung        ! Sung et al. identification(s) (G2)
      character*13  Note        ! 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

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

      integer*4     SST_1       ! Running identification number (G1)
      integer*4     RAh_1       ! (h) Hour of Right Ascension (J2000)
      integer*4     RAm_1       ! (min) Minute of Right Ascension (J2000)
      real*4        RAs_1       ! (s) Second of Right Ascension (J2000)
      character*1   DE__1       ! Sign of declination (J2000)
      integer*4     DEd_1       ! (deg) Degree of Declination (J2000)
      integer*4     DEm_1       ! (arcmin) Arcminute of Declination (J2000)
      real*4        DEs_1       ! (arcsec) Arcsecond of Declination (J2000)
      real*4        v_3_6__1    ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude
      real*4        v_4_5__1    ! (mag) Spitzer/IRAC 4.5 micron band magnitude
      real*4        v_5_8__1    ! (mag) ? Spitzer/IRAC 5.8 micron band magnitude
      real*4        v_8_0__1    ! (mag) ? Spitzer/IRAC 8.0 micron band magnitude
      real*4        v_24__1     ! (mag) ? Spitzer/MIPS 24 micron band magnitude
      real*4        e__3_6__1   ! (mag) ? Uncertainty in [3.6]
      real*4        e__4_5__1   ! (mag) Uncertainty in [4.5]
      real*4        e__5_8__1   ! (mag) ? Uncertainty in [5.8]
      real*4        e__8_0__1   ! (mag) ? Uncertainty in [8.0]
      real*4        e__24__1    ! (mag) ? Uncertainty in [24]
      integer*4     o__3_6__1   ! Number of [3.6] observations
      integer*4     o__4_5__1   ! Number of [4.5] observations
      integer*4     o__5_8__1   ! Number of [5.8] observations
      integer*4     o__8_0__1   ! Number of [8.0] observations
      integer*4     o__24__1    ! Number of [24] observations
      character*6   Class       ! Object classification (Galaxy, I, II or II/III)
      real*4        Signi       ! X-ray detection significance (1)
      real*4        Dist        ! (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       ! Running identification number (G1)
      character*1   f_SST       ! [a] long exposure images used (1)
      real*4        v_3_6_6     ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude on
*                                  2004 Mar 6
      real*4        e__3_6_6    ! (mag) ? Uncertainty in [3.6]
      real*4        v_3_6_8     ! (mag) ? Spitzer/IRAC 3.6 micron band magnitude on
*                                  2004 Oct 8
      real*4        e__3_6_8    ! (mag) ? Uncertainty in [3.6]
      real*4        d_3_6_      ! (mag) ? [3.6] difference
      real*4        v_4_5_6     ! (mag) ? Spitzer/IRAC [4.5 micron band magnitude on
*                                  2004 Mar 6
      real*4        e__4_5_6    ! (mag) ? Uncertainty in [4.5]
      real*4        v_4_5_8     ! (mag) ? Spitzer/IRAC 4.5 micron band magnitude on
*                                  2004 Oct 8
      real*4        e__4_5_8    ! (mag) ? Uncertainty in [4.5]
      real*4        d_4_5_      ! (mag) ? [4.5] difference
      character*6   Class_1     ! Infra-red classification (I, II or II/III)
      character*8   Other       ! Other classification (X or X+Halpha)
      character*13  OName       ! 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       ! Running identification number (G1)
      character*1   n_SST       ! [bc] Note on source (1)
      character*13  OName_1     ! Sung et al. identification(s) (G2)
      real*4        v_3_6__2    ! (mag) Spitzer/IRAC 3.6 micron band magnitude
      real*4        v_4_5__2    ! (mag) Spitzer/IRAC 4.5 micron band magnitude
      real*4        v_5_8__2    ! (mag) Spitzer/IRAC 5.8 micron band magnitude
      real*4        v_8_0__2    ! (mag) Spitzer/IRAC 8.0 micron band magnitude
      real*4        v_24__2     ! (mag) ? Spitzer/MIPS 24 micron band magnitude
      character*3   Ha_         ! [Yes/No/? ] H{alpha} emission?
      character*2   Class_2     ! IR classification (I or II)
      real*4        SED         ! SED slope
      real*4        e_SED       ! SED uncertainty
      real*4        Qcc         ! Mean value of a YSO class Q_CC_ (2)
      real*4        D_I         ! 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,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,21991
        read(1,'(A165)')ar__
        read(ar__,1)
     +  SST,RAh,RAm,RAs,DE_,DEd,DEm,DEs,v_3_6_,v_4_5_,v_5_8_,v_8_0_,
     +  v_24_,e__3_6_,e__4_5_,e__5_8_,e__8_0_,e__24_,o__3_6_,o__4_5_,
     +  o__5_8_,o__8_0_,o__24_,Dup,Mem,v2MASS,Sung,Note
        if(ar__(30:35) .EQ. '') v_3_6_ = rNULL__
        if(ar__(37:42) .EQ. '') v_4_5_ = rNULL__
        if(ar__(44:49) .EQ. '') v_5_8_ = rNULL__
        if(ar__(51:56) .EQ. '') v_8_0_ = rNULL__
        if(ar__(58:62) .EQ. '') v_24_ = rNULL__
        if(ar__(64:68) .EQ. '') e__3_6_ = rNULL__
        if(ar__(70:74) .EQ. '') e__4_5_ = rNULL__
        if(ar__(76:80) .EQ. '') e__5_8_ = rNULL__
        if(ar__(82:86) .EQ. '') e__8_0_ = rNULL__
        if(ar__(88:92) .EQ. '') e__24_ = rNULL__
        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)
     +  SST,RAh,RAm,RAs,DE_,DEd,DEm,DEs,v_3_6_,v_4_5_,v_5_8_,v_8_0_,
     +  v_24_,e__3_6_,e__4_5_,e__5_8_,e__8_0_,e__24_,o__3_6_,o__4_5_,
     +  o__5_8_,o__8_0_,o__24_,Dup,Mem,v2MASS,Sung,Note
        write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
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,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,43
        read(1,'(A117)')ar__1
        read(ar__1,2)
     +  SST_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,v_3_6__1,
     +  v_4_5__1,v_5_8__1,v_8_0__1,v_24__1,e__3_6__1,e__4_5__1,
     +  e__5_8__1,e__8_0__1,e__24__1,o__3_6__1,o__4_5__1,o__5_8__1,
     +  o__8_0__1,o__24__1,Class,Signi,Dist
        if(ar__1(29:34) .EQ. '') v_3_6__1 = rNULL__
        if(ar__1(43:48) .EQ. '') v_5_8__1 = rNULL__
        if(ar__1(50:55) .EQ. '') v_8_0__1 = rNULL__
        if(ar__1(57:61) .EQ. '') v_24__1 = rNULL__
        if(ar__1(63:67) .EQ. '') e__3_6__1 = rNULL__
        if(ar__1(75:79) .EQ. '') e__5_8__1 = rNULL__
        if(ar__1(81:85) .EQ. '') e__8_0__1 = rNULL__
        if(ar__1(87:91) .EQ. '') e__24__1 = rNULL__
        RAdeg_1 = rNULL__
        DEdeg_1 = 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 .GT. -180) RAdeg_1=RAh_1*15.
        if(RAm_1 .GT. -180) RAdeg_1=RAdeg_1+RAm_1/4.
        if(RAs_1 .GT. -180) RAdeg_1=RAdeg_1+RAs_1/240.
        if(DEd_1 .GE. 0) DEdeg_1=DEd_1
        if(DEm_1 .GE. 0) DEdeg_1=DEdeg_1+DEm_1/60.
        if(DEs_1 .GE. 0) DEdeg_1=DEdeg_1+DEs_1/3600.
        if(DE__1.EQ.'-'.AND.DEdeg_1.GE.0) DEdeg_1=-DEdeg_1
c    ..............Just test output...........
        write(6,2)
     +  SST_1,RAh_1,RAm_1,RAs_1,DE__1,DEd_1,DEm_1,DEs_1,v_3_6__1,
     +  v_4_5__1,v_5_8__1,v_8_0__1,v_24__1,e__3_6__1,e__4_5__1,
     +  e__5_8__1,e__8_0__1,e__24__1,o__3_6__1,o__4_5__1,o__5_8__1,
     +  o__8_0__1,o__24__1,Class,Signi,Dist
        write(6,'(6H Pos: 2F8.4)') RAdeg_1,DEdeg_1
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,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,28
        read(1,'(A102)')ar__2
        read(ar__2,3)
     +  SST_2,f_SST,v_3_6_6,e__3_6_6,v_3_6_8,e__3_6_8,d_3_6_,v_4_5_6,
     +  e__4_5_6,v_4_5_8,e__4_5_8,d_4_5_,Class_1,Other,OName
        if(ar__2(8:13) .EQ. '') v_3_6_6 = rNULL__
        if(ar__2(15:19) .EQ. '') e__3_6_6 = rNULL__
        if(ar__2(21:26) .EQ. '') v_3_6_8 = rNULL__
        if(ar__2(28:32) .EQ. '') e__3_6_8 = rNULL__
        if(ar__2(34:39) .EQ. '') d_3_6_ = rNULL__
        if(ar__2(41:46) .EQ. '') v_4_5_6 = rNULL__
        if(ar__2(48:52) .EQ. '') e__4_5_6 = rNULL__
        if(ar__2(54:59) .EQ. '') v_4_5_8 = rNULL__
        if(ar__2(61:65) .EQ. '') e__4_5_8 = rNULL__
        if(ar__2(67:72) .EQ. '') d_4_5_ = rNULL__
c    ..............Just test output...........
        write(6,3)
     +  SST_2,f_SST,v_3_6_6,e__3_6_6,v_3_6_8,e__3_6_8,d_3_6_,v_4_5_6,
     +  e__4_5_6,v_4_5_8,e__4_5_8,d_4_5_,Class_1,Other,OName
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,status='old',file=
     +'table5.dat')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,10
        read(1,'(A82)')ar__3
        read(ar__3,4)
     +  SST_3,n_SST,OName_1,v_3_6__2,v_4_5__2,v_5_8__2,v_8_0__2,
     +  v_24__2,Ha_,Class_2,SED,e_SED,Qcc,D_I
        if(ar__3(50:54) .EQ. '') v_24__2 = rNULL__
c    ..............Just test output...........
        write(6,4)
     +  SST_3,n_SST,OName_1,v_3_6__2,v_4_5__2,v_5_8__2,v_8_0__2,
     +  v_24__2,Ha_,Class_2,SED,e_SED,Qcc,D_I
c    .......End.of.Just test output...........
      end do
      close(1)

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