FORTRAN Generation
(/./ftp/cats/J/ApJ/699/L139)

Conversion of standardized ReadMe file for file /./ftp/cats/J/ApJ/699/L139 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-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/ApJ/699/L139           Spectral parameters of SNe Ia             (Wang+, 2009)
*================================================================================
*Improved distances to type Ia supernovae with two spectroscopic subclasses.
*    Wang X., Filippenko A.V., Ganeshalingam M., Li W., Silverman J.M., Wang L.,
*    Chornock R., Foley R.J., Gates E.L., Macomber B., Serduke F.J.D.,
*    Steele T.N., Wong D.S.
*   <Astrophys. J., 699, L139-L143 (2009)>
*   =2009ApJ...699L.139W
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table1.dat'	! Observed parameters of the SN Ia sample

      integer*4 nr__
      parameter (nr__=158)	! Number of records
      character*68 ar__   	! Full-size record

      character*6   SN         (nr__) ! Supernova identification (YYYYaa)
      character*1   f_SN       (nr__) ! [d] SN-Ia with Cepheid distance
      integer*4     cz         (nr__) ! (km/s) Recession velocity (2)
      real*4        VMAG       (nr__) ! (mag) Absolute V band magnitude at maximum
      real*4        e_VMAG     (nr__) ! (mag) The 1{sigma} uncertainty in VMAG
      real*4        Dm15       (nr__) ! (mag) Luminosity decline rate {Delta}m_15_ (3)
      real*4        e_Dm15     (nr__) ! (mag) The 1{sigma} uncertainty in Delm15
      real*4        B_V        (nr__) ! (mag) The (B-V) color index at maximum
      real*4        e_B_V      (nr__) ! (mag) The 1{sigma} uncertainty in B-V
      real*4        E_B_V      (nr__) ! (mag) Host galaxy (B-V) color excess
      real*4        e_E_B_V    (nr__) ! (mag) Uncertainty in E(B-V)
      real*4        TType      (nr__) ! ? RC3 host galaxy T morphology
      character*1   f_TType    (nr__) ! [?] Uncertainty flag on Morph
      character*2   Type       (nr__) ! SN type ("HV" or "N" for normal) (4)
*Note (2): Distances to the SNe are computed by using the redshifts of their
*     host galaxies, in the reference frame of the 3K cosmic microwave
*     background radiation for samples at redshift z{>~}0.01 or corrected 
*     to a self-consistent Virgocentric infall of 220km/s for closer ones,
*     with a Hubble constant H_0_=70.5 km/s/Mpc (Komatsu et al.
*     2009ApJS..180..330K). A peculiar-velocity component of 300km/s is
*     included in the distance-modulus uncertainties. Cepheid distances 
*     are adopted whenever available (see Wang X. et al. 2006, Cat.
*     J/ApJ/645/488 and references therein).
*Note (3): Value has been corrected for the reddening effect
*     (Phillips et al.  1999AJ....118.1766P).
*Note (4): SN Ia sample is divided into "Normal" and "HV" groups according
*     to the observed velocity of SiII{lambda}6355.
*   N = "Normal" group which consists of normal SNe Ia populating a narrow strip
*       in the SiII velocity distribution, with an average expansion velocity
*       <{nu}>=10600+/-400km/s near B maximum;
*  HV = the other group which consists of objects with higher velocities,
*       {nu}>~11800km/s.

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

C  Loading file 'table1.dat'	! Observed parameters of the SN Ia sample

C  Format for file interpretation

    1 format(
     +  A6,1X,A1,1X,I5,1X,F6.2,1X,F4.2,1X,F4.2,1X,F4.2,1X,F5.2,1X,
     +  F4.2,1X,F5.2,1X,F4.2,1X,F5.1,A1,1X,A2)

C  Effective file loading

      open(unit=1,status='old',file=
     +'table1.dat')
      write(6,*) '....Loading file: table1.dat'
      do i__=1,158
        read(1,'(A68)')ar__
        read(ar__,1)
     +  SN(i__),f_SN(i__),cz(i__),VMAG(i__),e_VMAG(i__),Dm15(i__),
     +  e_Dm15(i__),B_V(i__),e_B_V(i__),E_B_V(i__),e_E_B_V(i__),
     +  TType(i__),f_TType(i__),Type(i__)
        if(ar__(60:64) .EQ. '') TType(i__) = rNULL__
c    ..............Just test output...........
        write(6,1)
     +  SN(i__),f_SN(i__),cz(i__),VMAG(i__),e_VMAG(i__),Dm15(i__),
     +  e_Dm15(i__),B_V(i__),e_B_V(i__),E_B_V(i__),e_E_B_V(i__),
     +  TType(i__),f_TType(i__),Type(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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