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<H2><A NAME="SECTION001344000000000000000">
Format of the table for the absorption line model (ABSC.TBL)</A>
</H2>
<DIV ALIGN="CENTER">
<TABLE CELLPADDING=3>
<TR><TD ALIGN="LEFT"><U>INPUT</U></TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT"> </TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">Column</TD>
<TD ALIGN="LEFT">Name</TD>
<TD ALIGN="LEFT"> </TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">1</TD>
<TD ALIGN="LEFT">: IDENT</TD>
<TD ALIGN="LEFT">Identification of the transition</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">2</TD>
<TD ALIGN="LEFT">: NH</TD>
<TD ALIGN="LEFT">Column density in nb (atoms)/cm<SUP>2</SUP></TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">3</TD>
<TD ALIGN="LEFT">: POS</TD>
<TD ALIGN="LEFT">Position of the absorption in Å</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT">In the case of a doublet, indicate only the</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT">position of the reddest component; the other</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT">will be set automatically.</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">4</TD>
<TD ALIGN="LEFT">: BVAL</TD>
<TD ALIGN="LEFT">b parameter
<!-- MATH: $\left( \sqrt \frac {2kT}{m}
\right)$ -->
<IMG
WIDTH="45" HEIGHT="67" ALIGN="MIDDLE" BORDER="0"
SRC="img401.gif"
ALT="$\left( \sqrt \frac {2kT}{m}
\right)$">
in km/s</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">5</TD>
<TD ALIGN="LEFT">: TRANS</TD>
<TD ALIGN="LEFT">This number indicates the line number where</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT">the corresponding atomic transition is</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT">identified in table ABSP.</TD>
</TR>
<TR><TD ALIGN="LEFT"><U>OUTPUT</U></TD>
<TD ALIGN="CENTER"> </TD>
<TD ALIGN="LEFT"> </TD>
<TD ALIGN="LEFT"> </TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">6</TD>
<TD ALIGN="LEFT">: VELOCITY</TD>
<TD ALIGN="LEFT">velocity of the cloud with respect to the source.</TD>
</TR>
<TR><TD ALIGN="LEFT"> </TD>
<TD ALIGN="CENTER">7</TD>
<TD ALIGN="LEFT">: ZA</TD>
<TD ALIGN="LEFT">redshift of the cloud, relative to the observer.</TD>
</TR>
</TABLE></DIV>
Possibility for 50 absorption lines.
<P><P>
<BR>
<P>
<U>N.B.</U>
<BR>
<UL>
<LI>All the data should be entered in the table as real. [except : IDENT
(character)]
<LI>The unit for wavelength is Å (c.f. coefficient for the continuum and
the emission on absorption lines).
</UL>
<P>
<P>
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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
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