% @(#)hst_spec.hlq	19.1 (ESO-IPG) 02/25/03 14:28:42
%++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
%.COPYRIGHT  (c)  1996 European Southern Observatory
%.IDENT      hst_spec.hlq
%.AUTHOR     PB, IPG/ESO
%.KEYWORDS   MIDAS, help files, 
%.PURPOSE    On-line help file for the command: VERIFY/SPEC
%.VERSION    1.0  15-JAN-96 : Creation, PB
%----------------------------------------------------------------
\se
SECTION./SPEC
\es\co
HST/SPEC					      15-JAN-96  PB
\oc\su
HST/SPEC  fits_wave fits_flux table
	converts two HST FITS files providing wavelength and flux information
\us\pu
Purpose:    
            This command converts two HST FITS files providing
            wavelength and flux information into a Midas table. 
            The columns :WAVE and :FLUX carry the wavelength and 
            flux information. Additional columns :LAB0001 to :LABxxxx
            provide intermediate exposures. All descriptors from the
            flux FITS files are copied to the result table.
\up\sy
Syntax:     
            HST/SPEC  fits_wave fits_flux table
 \\
\ys\pa
            fits_wave   = Name of the wavelength FITS file
 \\
\ap\pa
            fits_flux   = Name of the flux FITS file
 \\
\ap\pa
            table       = Name of the result Midas table 
 \\
\ap\no
Note:       
            None.
 \\
\on\exs
Examples:
\ex
            HST/SPEC Y2AG0102T.C0F_29_CAL Y2AG0102T.C1F_29_CAL t102.tbl
\xe \sxe
