% @(#)computemis.hlq	17.1.1.1 (ESO-IPG) 01/25/02 17:13:44 
%++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++++
%.COPYRIGHT  (c)  1990 European Southern Observatory
%.IDENT      computemis.hlq
%.AUTHOR     MP, IPG/ESO
%.KEYWORDS   MIDAS, help files, COMPUTE/EMISSION
%.PURPOSE    On-line help file for the command: COMPUTE/EMISSION
%.VERSION    1.0  25-APR-1988 : Creation, MP
%----------------------------------------------------------------
\se
SECTION./EMISSION
\es\co
COMPUTE/EMISSION                                             25-APR-1988 MP
\oc\su
COMPUTE/EMISSION outframe [em_table]
	computes a synthetic 1dim.  emission spectrum
\us\pu
Purpose:   
           Creates a synthetic 1D spectrum  consisting of a polynomial
	   continuum and gaussian emission lines.
	   This image is to be used by the command COMPUTE/ABSORPTION.
\up\sub
Subject:   
           Spectroscopy, synthetic spectrum
\bus\sy
Syntax:    
           COMPUTE/EMISSION outframe [em_table]
\ys\pa
           outframe  = output synthetic spectrum
\ap\pa
           em_table  = table containing the line parameters.
                       A template can be found in \\
                       MID_CLOUD:emi.tbl
                       Default: indicates that no emission line will
		       be created
\ap\no
Note:      
           The coefficients for the continuum and the image dimensions.
	   are to be entered via keywords CLDCT and CLDDIM. For a complete 
           description see MIDAS Users Guide: CLOUD CONTEXT.
\on\exs
Examples:
\ex
           COMPUTE/EMISION backg line
\xe\sxe