Sophie

Sophie

distrib > Mageia > 5 > i586 > by-pkgid > 37ce2601040f8edc2329d4714238376a > files > 3987

eso-midas-doc-13SEPpl1.2-3.mga5.i586.rpm

<!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>Estimated parameters</TITLE>
<META NAME="description" CONTENT="Estimated parameters">
<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="node289.html">
<LINK REL="previous" HREF="node287.html">
<LINK REL="up" HREF="node286.html">
<LINK REL="next" HREF="node289.html">
</HEAD>
<BODY >
<!--Navigation Panel-->
<A NAME="tex2html5033"
 HREF="node289.html">
<IMG WIDTH="37" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="next"
 SRC="icons.gif/next_motif.gif"></A> 
<A NAME="tex2html5030"
 HREF="node286.html">
<IMG WIDTH="26" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="up"
 SRC="icons.gif/up_motif.gif"></A> 
<A NAME="tex2html5024"
 HREF="node287.html">
<IMG WIDTH="63" HEIGHT="24" ALIGN="BOTTOM" BORDER="0" ALT="previous"
 SRC="icons.gif/previous_motif.gif"></A> 
<A NAME="tex2html5032"
 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="tex2html5034"
 HREF="node289.html">Individual data</A>
<B> Up:</B> <A NAME="tex2html5031"
 HREF="node286.html">Final results</A>
<B> Previous:</B> <A NAME="tex2html5025"
 HREF="node287.html">Residual plots</A>
<BR>
<BR>
<!--End of Navigation Panel-->

<H3><A NAME="SECTION001857200000000000000">
Estimated parameters</A>
</H3>

<P>
After the last residual plot, the final parameter values
(and their errors) are printed, including
the magnitudes and colors of the individual stars in the extinction solution.
The errors for the color indices take account of the covariances between the
magnitudes.
This is followed by a table of the individual residuals, which includes the
symbols used to identify different stars in the residual plots.

<P>
<BR><HR>
<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
</ADDRESS>
</BODY>
</HTML>