<!DOCTYPE HTML PUBLIC "-//W3C//DTD HTML 3.2 Final//EN"> <!--Converted with LaTeX2HTML 98.1p1 release (March 2nd, 1998) originally by Nikos Drakos (nikos@cbl.leeds.ac.uk), CBLU, University of Leeds * revised and updated by: Marcus Hennecke, Ross Moore, Herb Swan * with significant contributions from: Jens Lippmann, Marek Rouchal, Martin Wilck and others --> <HTML> <HEAD> <TITLE>Format of the table for the emission line model (EMI.TBL)</TITLE> <META NAME="description" CONTENT="Format of the table for the emission line model (EMI.TBL)"> <META NAME="keywords" CONTENT="vol2"> <META NAME="resource-type" CONTENT="document"> <META NAME="distribution" CONTENT="global"> <META HTTP-EQUIV="Content-Type" CONTENT="text/html; charset=iso-8859-1"> <LINK REL="STYLESHEET" HREF="vol2.css"> <LINK REL="next" HREF="node196.html"> <LINK REL="previous" HREF="node194.html"> <LINK REL="up" HREF="node192.html"> <LINK REL="next" HREF="node196.html"> </HEAD> <BODY > <!--Navigation Panel--> <A NAME="tex2html3853" HREF="node196.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="icons.gif/next_motif.gif"></A> <A NAME="tex2html3850" HREF="node192.html"> <IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="icons.gif/up_motif.gif"></A> <A NAME="tex2html3844" HREF="node194.html"> <IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="icons.gif/previous_motif.gif"></A> <A NAME="tex2html3852" HREF="node1.html"> <IMG WIDTH="65" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="contents" SRC="icons.gif/contents_motif.gif"></A> <BR> <B> Next:</B> <A NAME="tex2html3854" HREF="node196.html">Format of the table</A> <B> Up:</B> <A NAME="tex2html3851" HREF="node192.html">Auxiliary Data</A> <B> Previous:</B> <A NAME="tex2html3845" HREF="node194.html">Format of the table</A> <BR> <BR> <!--End of Navigation Panel--> <H2><A NAME="SECTION001343000000000000000"> Format of the table for the emission line model (EMI.TBL)</A> </H2> The lines are assumed to be gaussian: <BR><P></P> <DIV ALIGN="CENTER"> <!-- MATH: \begin{displaymath} I(\lambda) = HMAX * EXP \left[-Ln2 \ \left( \frac{2(\lambda - POS)^{2}}{FWHM} \right)^{2}\right] \end{displaymath} --> <IMG WIDTH="486" HEIGHT="81" SRC="img400.gif" ALT="\begin{displaymath}I(\lambda) = HMAX * EXP \left[-Ln2 \ \left( \frac{2(\lambda - POS)^{2}}{FWHM} \right)^{2}\right] \end{displaymath}"> </DIV> <BR CLEAR="ALL"> <P></P> <DIV ALIGN="CENTER"> <TABLE CELLPADDING=3> <TR><TD ALIGN="CENTER">Column</TD> <TD ALIGN="LEFT">Name</TD> <TD ALIGN="LEFT"> </TD> </TR> <TR><TD ALIGN="CENTER">1</TD> <TD ALIGN="LEFT">IDENT</TD> <TD ALIGN="LEFT"> </TD> </TR> <TR><TD ALIGN="CENTER">2</TD> <TD ALIGN="LEFT">HMAX</TD> <TD ALIGN="LEFT">(Flux unit)</TD> </TR> <TR><TD ALIGN="CENTER">3</TD> <TD ALIGN="LEFT">POS</TD> <TD ALIGN="LEFT">(Ångstrom)</TD> </TR> <TR><TD ALIGN="CENTER">4</TD> <TD ALIGN="LEFT">FWHM</TD> <TD ALIGN="LEFT">(Ångstrom)</TD> </TR> </TABLE></DIV> <P> Possibility for 50 emission lines. <P> <BR><HR> <ADDRESS> <I>Petra Nass</I> <BR><I>1999-06-15</I> </ADDRESS> </BODY> </HTML>