mkoctfile problem

[bugsalad]

Hi everybody!

I tried to make a .oct-file from a  fortran-file, but had no success.
I get "error: `iau_SP00' undefined near line 2 column 1" when calling the
function.

* I started with the subroutine sp00.for from SOFA
(http://www.iau-sofa.rl.ac.uk/2008_0301/Downloads.html).
* I replaced all special Characters in sp00.for (\r\n to \n and such) and
renamed it to sp00.f (checked with vim)
* called from bash mkoctfile -o iau_SP00.oct sp00.f. This executed without
an error and returned the iau_SP00.oct-file
* started octave from bash
* added the path whit the .oct-file 
* tried to run it with and without parameters and always get the same error
(as above).

Thanks for any help!
Here is the sp00.for code:

      DOUBLE PRECISION FUNCTION iau_SP00 ( DATE1, DATE2 )
*+
*  - - - - - - - - -
*   i a u _ S P 0 0
*  - - - - - - - - -
*
*  The quantity s', positioning the Terrestrial Ephemeris Origin on the
*  equator of the Celestial Intermediate Pole.
*
*  This routine is part of the International Astronomical Union's
*  SOFA (Standards of Fundamental Astronomy) software collection.
*
*  Status:  canonical model.
*
*  Given:
*     DATE1,DATE2    d      TT as a 2-part Julian Date (Note 1)
*
*  Returned:
*     iau_SP00       d      the quantity s' in radians (Note 2)
*
*  Notes:
*
*  1) The TT date DATE1+DATE2 is a Julian Date, apportioned in any
*     convenient way between the two arguments.  For example,
*     JD(TT)=2450123.7 could be expressed in any of these ways,
*     among others:
*
*            DATE1          DATE2
*
*         2450123.7D0        0D0        (JD method)
*          2451545D0      -1421.3D0     (J2000 method)
*         2400000.5D0     50123.2D0     (MJD method)
*         2450123.5D0       0.2D0       (date & time method)
*
*     The JD method is the most natural and convenient to use in
*     cases where the loss of several decimal digits of resolution
*     is acceptable.  The J2000 method is best matched to the way
*     the argument is handled internally and will deliver the
*     optimum resolution.  The MJD method and the date & time methods
*     are both good compromises between resolution and convenience.
*
*  2) The quantity s' is obtained from polar motion observations by
*     numerical integration, and so is in essence unpredictable.
*     However, it is dominated by a secular drift of about
*     47 microarcseconds per century, which is the approximation
*     evaluated by the present routine.
*
*  Reference:
*
*     McCarthy, D. D., Petit, G. (eds.), IERS Conventions (2003),
*     IERS Technical Note No. 32, BKG (2004)
*
*  This revision:  2005 August 24
*
*  Copyright (C) 2005 IAU SOFA Review Board.  See notes at end.
*
*-----------------------------------------------------------------------

      IMPLICIT NONE

      DOUBLE PRECISION DATE1, DATE2

*  Arcseconds to radians
      DOUBLE PRECISION DAS2R
      PARAMETER ( DAS2R = 4.848136811095359935899141D-6 )

*  Reference epoch (J2000), JD
      DOUBLE PRECISION DJ0
      PARAMETER ( DJ0 = 2451545D0 )

*  Days per Julian century
      DOUBLE PRECISION DJC
      PARAMETER ( DJC = 36525D0 )

*  Time since J2000, in Julian centuries
      DOUBLE PRECISION T

* - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - -

*  Interval between fundamental epoch J2000.0 and current date (JC).
      T = ( ( DATE1-DJ0 ) + DATE2 ) / DJC

*  Approximate S'.
      iau_SP00 = -47D-6 * T * DAS2R

*  Finished.

*+----------------------------------------------------------------------
*
*  Copyright (C) 2005
*  Standards Of Fundamental Astronomy Review Board
*  of the International Astronomical Union.
*
*  =====================
*  SOFA Software License
*  =====================
*
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*
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*
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*-----------------------------------------------------------------------

      END


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