FORTRAN Generation
(/./ftp/cats/J/A_A/534/A118)

Conversion of standardized ReadMe file for file /./ftp/cats/J/A_A/534/A118 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_1.5, on 2013-May-24
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__=-1.e37)     	! NULL real number
      parameter  (iNULL__=-2147483647)	! NULL int  number

C=============================================================================
Cat. J/A+A/534/A118   Predicted dust emissivity in 100-10000um bands (Paradis+, 2011)
*================================================================================
*Far-infrared to millimeter astrophysical dust emission.
*II. Comparison of the model with astronomical data.
*    Paradis D, Bernard J.P., Meny C., Gromov V.
*   <Astron. Astrophys. 534, A118 (2011)>
*   =2011A&A...534A.118P
C=============================================================================

C  Internal variables

      integer*4 i__

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

C  Declarations for 'table5.dat'	! Predicted emissivities as a function of temperature
                            in the IRAS, Herschel, and Planck photometric bands

      integer*4 nr__
      parameter (nr__=8)	! Number of records
      character*129 ar__   	! Full-size record

      integer*4     Td         (nr__) ! (K) [5/100] Dust temperature
      real*4        e100I      (nr__) ! (cm2) Predicted emissivity in the IRAS 100um band (1)
      real*4        e160P      (nr__) ! (cm2) Predicted emissivity in the PACS 160um band (1)
      real*4        e250S      (nr__) ! (cm2) Predicted emissivity in the SPIRE 250um band (1)
      real*4        e350S      (nr__) ! (cm2) Predicted emissivity in the SPIRE 350um band (1)
      real*4        e350H      (nr__) ! (cm2) Predicted emissivity in the HFI 350um band (1)
      real*4        e500S      (nr__) ! (cm2) Predicted emissivity in the SPIRE 500um band (1)
      real*4        e550H      (nr__) ! (cm2) Predicted emissivity in the HFI 550um band (1)
      real*4        e850H      (nr__) ! (cm2) Predicted emissivity in the HFI 850um band (1)
      real*4        e1382H     (nr__) ! (cm2) Predicted emissivity in the HFI 1382um band (1)
      real*4        e2096H     (nr__) ! (cm2) Predicted emissivity in the HFI 2096um band (1)
      real*4        e2998H     (nr__) ! (cm2) Predicted emissivity in the HFI 2998um band (1)
      real*4        e4286L     (nr__) ! (cm2) Predicted emissivity in the LFI 4296um band (1)
      real*4        e6818L     (nr__) ! (cm2) Predicted emissivity in the LFI 6818um band (1)
      real*4        e10000L    (nr__) ! (cm2) Predicted emissivity in the LFI 10000um band (1)
*Note (1): Emissivities normalized to 10^-25^cm^2^/N_H_, at 250um for a
*          temperature of 17.5K.

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

C  Loading file 'table5.dat'	! Predicted emissivities as a function of temperature
*                            in the IRAS, Herschel, and Planck photometric bands

C  Format for file interpretation

    1 format(
     +  I3,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,
     +  E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2,1X,E8.2)

C  Effective file loading

      open(unit=1,file='table5.dat', status='old')
      write(6,*) '....Loading file: table5.dat'
      do i__=1,8
        read(1,'(A129)')ar__
        read(ar__,1)
     +  Td(i__),e100I(i__),e160P(i__),e250S(i__),e350S(i__),
     +  e350H(i__),e500S(i__),e550H(i__),e850H(i__),e1382H(i__),
     +  e2096H(i__),e2998H(i__),e4286L(i__),e6818L(i__),e10000L(i__)
c    ..............Just test output...........
        write(6,1)
     +  Td(i__),e100I(i__),e160P(i__),e250S(i__),e350S(i__),
     +  e350H(i__),e500S(i__),e550H(i__),e850H(i__),e1382H(i__),
     +  e2096H(i__),e2998H(i__),e4286L(i__),e6818L(i__),e10000L(i__)
c    .......End.of.Just test output...........
      end do
      close(1)

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