FORTRAN Generation
(/./ftp/cats/J/ApJ/648/7)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/648/7 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-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/648/7 Ly{alpha} emitters at z=6.5 in Subaru Deep Field  (Kashikawa+, 2006)
*================================================================================
*The end of the reionization epoch probed by Ly{alpha} emitters at z = 6.5 in the
*Subaru Deep Field.
*    Kashikawa N., Shimasaku K., Malkan M.A., Doi M., Matsuda Y., Ouchi M.,
*    Taniguchi Y., Ly C., Nagao T., Iye M., Motohara K., Murayama T.,
*    Murozono K., Nariai K., Ohta K., Okamura S., Sasaki T., Shioya Y.,
*    Umemura M.
*   <Astrophys. J., 648, 7-22 (2006)>
*   =2006ApJ...648....7K
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table2.dat'	! Spectroscopic Properties of z=6.5 LAEs

      integer*4 nr__
      parameter (nr__=8)	! Number of records
      character*67 ar__   	! Full-size record

      integer*4     v_TAN2005_ (nr__) ! Sequential number
      character*16  SDF        (nr__) ! SDF designation (JHHMMSS.s+DDMMSS)
      real*4        z          (nr__) ! Redshift (1)
      real*4        F_Lya      (nr__) ! (10-21W/m2) Observed line flux in Ly{alpha} (2)
      real*4        L_Lya      (nr__) ! (10+35W) Estimated Ly{alpha} luminosity (3)
      real*4        SFR_Lya    (nr__) ! (solMass/yr) Ly{alpha} Stellar Formation Rate (3)(4)
      real*4        FWHM       (nr__) ! (0.1nm) FWHM in Angstroem (5)
      integer*4     FWHM2      (nr__) ! (km/s) FWHM in km/s (5)
      real*4        Sw         (nr__) ! (0.1nm) ? Weighted skewness (quantifies the
*                                       asymmetry of the emission lines)
      real*4        e_Sw       (nr__) ! (0.1nm) rms uncertainty on Sw
      character*1   Obs        (nr__) ! [FD] Observed with FOCAS (F) or DEIMOS (D)
*Note (1): The redshift was derived from the wavelength of the flux peak in
*     an observed spectrum assuming the rest wavelength of Ly{alpha} to be
*     1215{AA}. These measurements could be overestimated in the case of
*     significant damping wings by IGM. Also, the observed peak position was
*     slightly shifted redward due to instrumental resolution. See Fig. 9.
*Note (2): The observed line flux corresponds to the total amount.
*Note (3): No dust absorption correction was applied.
*Note (4): Estimated from the observed luminosities with the relation.
*     SFR(Lya)=9.1x10^-43^L(Lya)M_{sun}_/yr as in Taniguchi et al. (2005,
*     Cat. <J/PASJ/57/165>).
*Note (5): Corrected for instrumental broadening.

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

C  Loading file 'table2.dat'	! Spectroscopic Properties of z=6.5 LAEs

C  Format for file interpretation

    1 format(
     +  I2,5X,A16,1X,F5.3,1X,F5.2,1X,F4.2,1X,F4.2,1X,F4.1,1X,I3,1X,
     +  F5.2,1X,F4.2,1X,A1)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table2.dat')
      write(6,*) '....Loading file: table2.dat'
      do i__=1,8
        read(1,'(A67)')ar__
        read(ar__,1)
     +  v_TAN2005_(i__),SDF(i__),z(i__),F_Lya(i__),L_Lya(i__),
     +  SFR_Lya(i__),FWHM(i__),FWHM2(i__),Sw(i__),e_Sw(i__),Obs(i__)
        if(ar__(56:60) .EQ. '') Sw(i__) = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  v_TAN2005_(i__),SDF(i__),z(i__),F_Lya(i__),L_Lya(i__),
     +  SFR_Lya(i__),FWHM(i__),FWHM2(i__),Sw(i__),e_Sw(i__),Obs(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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