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%.COPYRIGHT  (c)  1993-2010 European Southern Observatory
%.IDENT      integrlong.hlq
%.AUTHOR     01-APR-93, IPG/ESO
%.KEYWORDS   MIDAS, help files, 
%.PURPOSE    On-line help file for the command: INTEGRATE/LONG
%.VERSION    1.0  PB : Creation, 01-APR-93
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SECTION./LONG
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INTEGRATE/LONG					   PB  25-OCT-10
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INTEGRATE/LONG  std  [flux]  [resp]
	Generates an intermediate response table from a standard star spectrum
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Purpose:    
            The reduced spectrum of a standard star (after extraction and
            rebinning) is compared to a flux table to generate the response
            table. This table must be processed further with RESPONSE/LONG
            to generate the final response image.
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Syntax:     
            INTEGRATE/LONG  std  [flux]  [resp]
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            std    = one-dimensional reduced spectrum of a standard star.
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            flux   = Flux table of the standard star. A collection of
                     flux tables is available in MID_FLUX. \\
                     Session keyword : FLUXTAB; no default value
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            resp   = Output response table.
                     Session keyword : RESPTAB; default: resp.tbl
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See also: 
            EXTINCTION/LONG, RESPONSE/LONG, RESPONSE/FILTER, PLOT/FLUX, \\
            PLOT/RESPONSE, CALIBRATE/FLUX
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Note:       
            The values of :BIN_W must be equal to the difference of
	    adjacent :WAVE entries! 
	    Furthermore, :BIN_W must be significantly larger than the 
	    stepsize of the spectrum, at least by a factor of 8.
	    E.g. in the tutorial, the stepsize is 2.0 and :BIN_W is 80.0
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Examples:
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            INTEGRATE/LONG  sp23  l745x4  
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