FORTRAN Generation
(/./ftp/cats/J/AJ/152/115)

Conversion of standardized ReadMe file for file /./ftp/cats/J/AJ/152/115 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-18
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/152/115    Pleiades members with K2 light curves. III.    (Stauffer+, 2016)
*================================================================================
*Rotation in the Pleiades with K2. III. Speculations on origins and evolution.
*    Stauffer J., Rebull L., Bouvier J., Hillenbrand L.A., Collier-Cameron A.,
*    Pinsonneault M., Aigrain S., Barrado D., Bouy H., Ciardi D., Cody A.M.,
*    David T., Micela G., Soderblom D., Somers G., Stassun K.G., Valenti J.,
*    Vrba F.J.
*    <Astron. J. 152, 115 (2016)>
*    =2016AJ....152..115S   (SIMBAD/NED BibCode)
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table3.dat'	! Derived data for Pleiades members with K2 light
                                  curves

      integer*4 nr__
      parameter (nr__=852)	! Number of records
      character*79 ar__   	! Full-size record

      integer*4     EPIC        ! Ecliptic Plane Input Catalog number
      character*23  Name        ! Source identifier
      real*4        Ksmag       ! (mag) [3.77/15.53] Apparent Ks band Vega magnitude
      real*4        v_V_K_0     ! (mag) [-9.11/9.21] Dereddened (V-Ks) color index
*                              (V-K_s_)_0_
      real*4        Mass        ! (Msun) [0.08/1.51]?=-9.99 Stellar mass
      real*4        Mbol        ! (mag) [1.08/11.3]?=-9 Bolometric magnitude (1)
      real*4        Rad         ! (Rsun) [0.19/2.37]?=-9 Stellar radius (1)
      integer*4     Teff        ! (K) [2823/8879]?=-9 Estimated effective temperature (2)
      real*4        DVmag       ! [-1.11/2.13]?=-9.99 Binary V band magnitude
*                              difference ({Delta}V)
      real*4        E_B_V       ! (mag) [0.22/0.53]? The (B-V) color excess (3)
*Note (1): We adopted the Pecaut & Mamajek 2013 (Cat. J/ApJS/208/9) bolometric
*     corrections to estimate MBol, and then the Stefan-Boltzmann law to estimate
*     radii.
*Note (2): The effective temperature estimates are based on the Pecaut & Mamajek
*     2013 (Cat. J/ApJS/208/9) Table5 data for main sequence stars, using B-V to
*     estimate Teff for the bluest stars and (V-K_s_) to estimate Teff for the
*     reddest stars, and a weighted average of the two estimates for G and K
*     dwarfs.
*Note (3): Given for stars with significantly larger reddening that the rest
*     which have to be treated separately.

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

C  Loading file 'table3.dat'	! Derived data for Pleiades members with K2 light
*                                  curves

C  Format for file interpretation

    1 format(
     +  I9,1X,A23,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,F5.2,1X,I4,1X,
     +  F5.2,1X,F4.2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table3.dat')
      write(6,*) '....Loading file: table3.dat'
      do i__=1,852
        read(1,'(A79)')ar__
        read(ar__,1)
     +  EPIC,Name,Ksmag,v_V_K_0,Mass,Mbol,Rad,Teff,DVmag,E_B_V
        if(ar__(76:79) .EQ. '') E_B_V = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  EPIC,Name,Ksmag,v_V_K_0,Mass,Mbol,Rad,Teff,DVmag,E_B_V
c    .......End.of.Just test output...........
      end do
      close(1)

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