<!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>Example</TITLE> <META NAME="description" CONTENT="Example"> <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="node200.html"> <LINK REL="previous" HREF="node198.html"> <LINK REL="up" HREF="node176.html"> <LINK REL="next" HREF="node200.html"> </HEAD> <BODY > <!--Navigation Panel--> <A NAME="tex2html3895" HREF="node200.html"> <IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next" SRC="icons.gif/next_motif.gif"></A> <A NAME="tex2html3892" HREF="node176.html"> <IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up" SRC="icons.gif/up_motif.gif"></A> <A NAME="tex2html3886" HREF="node198.html"> <IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous" SRC="icons.gif/previous_motif.gif"></A> <A NAME="tex2html3894" 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="tex2html3896" HREF="node200.html">Acknowledgements</A> <B> Up:</B> <A NAME="tex2html3893" HREF="node176.html">Inter-stellar/galactic Absorption Line Modelling</A> <B> Previous:</B> <A NAME="tex2html3887" HREF="node198.html">References</A> <BR> <BR> <!--End of Navigation Panel--> <H1><A NAME="SECTION001370000000000000000"> Example</A> </H1> <P> A concrete application is displayed step by step by the command: <TT>TUTORIAL/CLOUD</TT>. <P> The data used for this example are CaII absorption features observed in the spectrum of SN 1986g in NGC 5128 (observer: S. d'Odorico, instrument: CASPEC). <P> The two images (components K and H) have been pre-reduced so that the continuum is normalised to 1. Sampling is 0.05Å per pixel and the measured instrumental resolution, 17km/s. <P> The final cloud model consists of 12 absorption doublets. The corresponding image includes both components K and H and has been convolved by a gaussian PSF of 0.22Å (17km/s) FWHM. (The results are consistent with those derived by the ALAS software). <P> <P> <BR><HR> <ADDRESS> <I>Petra Nass</I> <BR><I>1999-06-15</I> </ADDRESS> </BODY> </HTML>
