FORTRAN Generation
(/./ftp/cats/J/A_A/416/281)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/416/281 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-28
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/A+A/416/281       X-ray spectra of 4 cool stars          (Sanz-forcada+, 2004)
*================================================================================
*Coronal versus photospheric abundances of stars with different activity levels.
*    Sanz-forcada J., Favata F., Micela G.
*   <Astron. Astrophys., 416, 281-290 (2004)>
*   =2004A&A...416..281S
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table4.dat'	! Chandra/LETG line fluxes of Procyon (6/7-Nov-1999)

      integer*4 nr__
      parameter (nr__=146)	! Number of records
      character*135 ar__   	! Full-size record

      character*8   Ion         ! Ion
      real*8        lambda      ! (0.1nm) Wavelength of the line as identified in the
*                                model.
      real*4        logTmax     ! ([K]) ? Maximum temperature of formation of the line
*                                  (unweighted by the Emission Measure
*                                  Distribution)
      real*4        Fobs        ! (mW/m2) Observed line flux
      real*4        S_N         ! Signal-to-noise ratio
      real*4        Ratio       ! ? log(observed flux/predicted flux) (1)
      character*94  Blends      ! Blends to the main line amounting more than a
*                                5% of the total flux (2)
*Note (1): The fluxes are in ergs units. Predicted flux includes
*    correction by interstellar medium absorption.
*Note (2): For some lines not identified in Astrophysical Plasma
*    Emission Model, a tentative identification is suggested in this column
*    based on Kelly (1987, Atomic and ionic spectrum lines below 2000
*    Angstroms. Hydrogen through Krypton (New York: American Institute of
*    Physics, Amer. Chem. Soc. and the Nat. Bureau of Standards)).

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

C  Declarations for 'table5.dat'	! Chandra/LETG line fluxes of epsilon Eri (7-Nov-1999)

      integer*4 nr__1
      parameter (nr__1=119)	! Number of records
      character*135 ar__1  	! Full-size record

      character*8   Ion_1       ! Ion
      real*8        lambda_1    ! (0.1nm) Wavelength of the line as identified in the
*                                model.
      real*4        logTmax_1   ! ([K]) ? Maximum temperature of formation of the line
*                                  (unweighted by the Emission Measure
*                                  Distribution)
      real*4        Fobs_1      ! (mW/m2) Observed line flux
      real*4        S_N_1       ! Signal-to-noise ratio
      real*4        Ratio_1     ! ? log(observed flux/predicted flux) (1)
      character*94  Blends_1    ! Blends to the main line amounting more than a
*                                5% of the total flux (2)
*Note (1): The fluxes are in ergs units. Predicted flux includes
*    correction by interstellar medium absorption.
*Note (2): For some lines not identified in Astrophysical Plasma
*    Emission Model, a tentative identification is suggested in this column
*    based on Kelly (1987, Atomic and ionic spectrum lines below 2000
*    Angstroms. Hydrogen through Krypton (New York: American Institute of
*    Physics, Amer. Chem. Soc. and the Nat. Bureau of Standards)).

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

C  Declarations for 'table6.dat'	! Chandra/HETG line fluxes of lambda And (21-Mar-2001)

      integer*4 nr__2
      parameter (nr__2=148)	! Number of records
      character*135 ar__2  	! Full-size record

      character*8   Ion_2       ! Ion
      real*8        lambda_2    ! (0.1nm) Wavelength of the line as identified in the
*                                model.
      real*4        logTmax_2   ! ([K]) ? Maximum temperature of formation of the line
*                                  (unweighted by the Emission Measure
*                                  Distribution)
      real*4        Fobs_2      ! (mW/m2) Observed line flux
      real*4        S_N_2       ! Signal-to-noise ratio
      real*4        Ratio_2     ! ? log(observed flux/predicted flux) (1)
      character*94  Blends_2    ! Blends to the main line amounting more than a
*                                5% of the total flux (2)
*Note (1): The fluxes are in ergs units. Predicted flux includes
*    correction by interstellar medium absorption.
*Note (2): For some lines not identified in Astrophysical Plasma
*    Emission Model, a tentative identification is suggested in this column
*    based on Kelly (1987, Atomic and ionic spectrum lines below 2000
*    Angstroms. Hydrogen through Krypton (New York: American Institute of
*    Physics, Amer. Chem. Soc. and the Nat. Bureau of Standards)).

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

C  Declarations for 'table7.dat'	! XMM/RGS line fluxes of V851 Cen (7-Mar-2003)

      integer*4 nr__3
      parameter (nr__3=51)	! Number of records
      character*135 ar__3  	! Full-size record

      character*8   Ion_3       ! Ion
      real*8        lambda_3    ! (0.1nm) Wavelength of the line as identified in the
*                                model.
      real*4        logTmax_3   ! ([K]) ? Maximum temperature of formation of the line
*                                  (unweighted by the Emission Measure
*                                  Distribution)
      real*4        Fobs_3      ! (mW/m2) Observed line flux
      real*4        S_N_3       ! Signal-to-noise ratio
      real*4        Ratio_3     ! ? log(observed flux/predicted flux) (1)
      character*94  Blends_3    ! Blends to the main line amounting more than a
*                                5% of the total flux (2)
*Note (1): The fluxes are in ergs units. Predicted flux includes
*    correction by interstellar medium absorption.
*Note (2): For some lines not identified in Astrophysical Plasma
*    Emission Model, a tentative identification is suggested in this column
*    based on Kelly (1987, Atomic and ionic spectrum lines below 2000
*    Angstroms. Hydrogen through Krypton (New York: American Institute of
*    Physics, Amer. Chem. Soc. and the Nat. Bureau of Standards)).

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

C  Loading file 'table4.dat'	! Chandra/LETG line fluxes of Procyon (6/7-Nov-1999)

C  Format for file interpretation

    1 format(A8,F8.4,1X,F3.1,1X,E8.3,1X,F4.1,1X,F5.2,1X,A94)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table4.dat')
      write(6,*) '....Loading file: table4.dat'
      do i__=1,146
        read(1,'(A135)')ar__
        read(ar__,1)Ion,lambda,logTmax,Fobs,S_N,Ratio,Blends
        if(ar__(18:20) .EQ. '') logTmax = rNULL__
        if(ar__(36:40) .EQ. '') Ratio = rNULL__
c    ..............Just test output...........
        write(6,1)Ion,lambda,logTmax,Fobs,S_N,Ratio,Blends
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table5.dat'	! Chandra/LETG line fluxes of epsilon Eri (7-Nov-1999)

C  Format for file interpretation

    2 format(A8,F8.4,1X,F3.1,1X,E8.3,1X,F4.1,1X,F5.2,1X,A94)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table5.dat')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,119
        read(1,'(A135)')ar__1
        read(ar__1,2)
     +  Ion_1,lambda_1,logTmax_1,Fobs_1,S_N_1,Ratio_1,Blends_1
        if(ar__1(18:20) .EQ. '') logTmax_1 = rNULL__
        if(ar__1(36:40) .EQ. '') Ratio_1 = rNULL__
c    ..............Just test output...........
        write(6,2)
     +  Ion_1,lambda_1,logTmax_1,Fobs_1,S_N_1,Ratio_1,Blends_1
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table6.dat'	! Chandra/HETG line fluxes of lambda And (21-Mar-2001)

C  Format for file interpretation

    3 format(A8,F8.4,1X,F3.1,1X,E8.3,1X,F4.1,1X,F5.2,1X,A94)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table6.dat')
      write(6,*) '....Loading file: table6.dat'
      do i__=1,148
        read(1,'(A135)')ar__2
        read(ar__2,3)
     +  Ion_2,lambda_2,logTmax_2,Fobs_2,S_N_2,Ratio_2,Blends_2
        if(ar__2(18:20) .EQ. '') logTmax_2 = rNULL__
        if(ar__2(36:40) .EQ. '') Ratio_2 = rNULL__
c    ..............Just test output...........
        write(6,3)
     +  Ion_2,lambda_2,logTmax_2,Fobs_2,S_N_2,Ratio_2,Blends_2
c    .......End.of.Just test output...........
      end do
      close(1)

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

C  Loading file 'table7.dat'	! XMM/RGS line fluxes of V851 Cen (7-Mar-2003)

C  Format for file interpretation

    4 format(A8,F8.4,1X,F3.1,1X,E8.3,1X,F4.1,1X,F5.2,1X,A94)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table7.dat')
      write(6,*) '....Loading file: table7.dat'
      do i__=1,51
        read(1,'(A135)')ar__3
        read(ar__3,4)
     +  Ion_3,lambda_3,logTmax_3,Fobs_3,S_N_3,Ratio_3,Blends_3
        if(ar__3(18:20) .EQ. '') logTmax_3 = rNULL__
        if(ar__3(36:40) .EQ. '') Ratio_3 = rNULL__
c    ..............Just test output...........
        write(6,4)
     +  Ion_3,lambda_3,logTmax_3,Fobs_3,S_N_3,Ratio_3,Blends_3
c    .......End.of.Just test output...........
      end do
      close(1)

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