FORTRAN Generation
(/./ftp/cats/J/ApJ/669/L33)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/669/L33 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-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/ApJ/669/L33    H{alpha} emission sources in h and {chi} Per  (Currie+, 2007)
*================================================================================
*Discovery of gas accretion onto stars in 13 Myr old h and {chi} Persei.
*    Currie T., Kenyon S.J., Balog Z., Bragg A., Tokarz S.
*   <Astrophys. J., 669, L33-L36 (2007)>
*   =2007ApJ...669L..33C
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! H{alpha} emission sources

      integer*4 nr__
      parameter (nr__=30)	! Number of records
      character*66 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     RAh         ! (h) Hour of Right Ascension (J2000) (1)
      integer*4     RAm         ! (min) Minute of Right Ascension (J2000) (1)
      real*4        RAs         ! (s) Second of Right Ascension (J2000) (1)
      character*1   DE_         ! Sign Declination (J2000) (1)
      integer*4     DEd         ! (deg) Degree of Declination (J2000) (1)
      integer*4     DEm         ! (arcmin) Arcminute of Declination (J2000) (1)
      real*4        DEs         ! (arcsec) Arcsecond of Declination (J2000) (1)
      character*4   SpType      ! Spectral type
      real*4        e_SpType    ! 1{sigma} error in the subclass of SpType
      real*4        EWHa        ! (0.1nm) H{alpha} equivalent width in Angstroms (2)
      character*1   Acc_        ! [yn] Accreting?
      real*4        Jmag        ! (mag) 2MASS J band magnitude (3)
      real*4        Kmag        ! (mag) 2MASS K_s_ band magnitude  (3)
      real*4        K_3_6       ! (mag) ? The (2MASS K_s_- IRAC 3.6 micron) color (3)
      real*4        K_8         ! (mag) ? The (2MASS K_s_- IRAC 8 micron) color (3)
*Note (1): Sources identified as [CKB2007] JHHMMSS.ss+DDMMSS.s in Simbad
*Note (2): Accreting sources have a H{alpha} equivalent width >=5{AA}.
*     All sources but the final entry are from Hectospec. 
*     Uncertainties were ~1-2{AA}.
*Note (3): All photometric measurements listed are 5{sigma} detections.
*     Sources were typically brighter than the 10{sigma} limit in J (15.7)
*     and K_s_ (14.8). See Currie et al. (2007, Cat. J/ApJ/659/599) for
*     typical the error distributions in each band.

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

C  Loading file 'table1.dat'	! H{alpha} emission sources

C  Format for file interpretation

    1 format(
     +  I1,1X,I2,1X,F5.2,A1,I2,1X,I2,1X,F4.1,1X,A4,1X,F4.2,1X,F5.2,1X,
     +  A1,1X,F6.3,1X,F6.3,1X,F5.3,1X,F6.3)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,30
        read(1,'(A66)')ar__
        read(ar__,1)
     +  RAh,RAm,RAs,DE_,DEd,DEm,DEs,SpType,e_SpType,EWHa,Acc_,Jmag,
     +  Kmag,K_3_6,K_8
        if(ar__(55:59) .EQ. '') K_3_6 = rNULL__
        if(ar__(61:66) .EQ. '') K_8 = 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)
     +  RAh,RAm,RAs,DE_,DEd,DEm,DEs,SpType,e_SpType,EWHa,Acc_,Jmag,
     +  Kmag,K_3_6,K_8
        write(6,'(6H Pos: 2F8.4)') RAdeg,DEdeg
c    .......End.of.Just test output...........
      end do
      close(1)

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