<!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>Summary of the parameters handled by the user:</TITLE> <META NAME="description" CONTENT="Summary of the parameters handled by the user:"> <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="previous" HREF="node180.html"> <LINK REL="up" HREF="node179.html"> <LINK REL="next" HREF="node184.html"> </HEAD> <BODY > <!--Navigation Panel--> <A NAME="tex2html3712" HREF="node184.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="icons.gif/next_motif.gif"></A> <A NAME="tex2html3709" HREF="node179.html"> <IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="icons.gif/up_motif.gif"></A> <A NAME="tex2html3705" HREF="node182.html"> <IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="icons.gif/previous_motif.gif"></A> <A NAME="tex2html3711" 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="tex2html3713" HREF="node184.html">Typical Run</A> <B> Up:</B> <A NAME="tex2html3710" HREF="node179.html">Astrophysical Context</A> <B> Previous:</B> <A NAME="tex2html3706" HREF="node182.html">Broadening Function</A> <BR> <BR> <!--End of Navigation Panel--> <H2><A NAME="SECTION001322000000000000000"> Summary of the parameters handled by the user:</A> </H2> <P> <U>INPUT</U> <P> <UL> <LI>Z source. <LI>The user is supposed to have determined the continuum and the emission line characteristics. <LI>Atomic data, for each transition <UL> <LI>SAKL = <!-- MATH: $\sum a_{kl}$ --> <IMG WIDTH="12" HEIGHT="42" ALIGN="MIDDLE" BORDER="0" SRC="img372.gif" ALT="$\sum a_{kl}$"> <LI> <!-- MATH: $\lambda_{kl}$ --> <IMG WIDTH="58" HEIGHT="72" ALIGN="MIDDLE" BORDER="0" SRC="img373.gif" ALT="$\lambda_{kl}$"> <LI>f<SUB><I>kl</I></SUB> <LI>g<SUB><I>l</I></SUB> <LI>g<SUB><I>k</I></SUB></UL> <LI>For each absorption line <UL> <LI>N <LI>b <LI>P (<IMG WIDTH="42" HEIGHT="56" ALIGN="BOTTOM" BORDER="0" SRC="img375.gif" ALT="$\lambda$">) : position Ångstroms of the observed absorption feature. </UL></UL> <P> <U>OUTPUT</U> <P> <UL> <LI><I>Z</I><SUB><I>a</I></SUB> <LI>v<SUB><I>rel</I></SUB></UL> <P> <P><P> <BR> <P><P> <BR> <P> <BR><HR> <ADDRESS> <I>Petra Nass</I> <BR><I>1999-06-15</I> </ADDRESS> </BODY> </HTML>