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<H2><A NAME="SECTION001031000000000000000">
Detecting and Identifying Arc Lines</A>
</H2>

<P>
For optimum results, it is important to use a comparison spectrum with
as high a signal-to-noise ratio of the lines as possible.  It is
therefore advisible to flat-field<A NAME="5769">&#160;</A> also the arc
spectrum in order to correct for small-scale fluctuations. Another
good idea is to filter the frame along the slit using the command <TT>FILTER/MEDIAN</TT> with a rectangular filter window of one pixel in the
dispersion direction and several pixels in the perpendicular
direction. For the row-by-row method one could also consider smoothing
the spectra along the slit axis which would provide for a stronger
coupling between neighbouring rows and thereby yield a solution which
is intermediate between the extremes presented by the two pure
methods.

<P>
<UL>
<P>
<LI><TT>SEARCH/LONG:</TT> Finds the positions of reference lines in world coordinates.
Positions are by default estimated by the center of fitted Gaussians.
Other centering methods are available (Gravity, Maximum) but could
result in systematic position errors  (See Hensberge &amp; Verschueren, 
Messenger, <B>58</B>, 51).
The results are stored in a table called <TT>line.tbl</TT>. 
The parameter <TT>YWIND</TT> corresponds the half-size of the row 
averaging window applied to adjacent rows of the spectrum for an
improvement of the signal to noise ratio. The parameter <TT>YSTEP</TT>
controls the step in rows between successive arc line detections. The
value <TT>YSTEP=1</TT> corresponds to the default row-by-row method and larger
values can be used to get a quicker calibration. The algorithm detects 
lines whose strength exceeds a certain threshold (parameter <TT>THRES</TT>) 
above the local background. The local background
results from a median estimate performed on a sliding window which 
size is controlled by the parameter <TT>WIDTH</TT>. The command
<TT>PLOT/SEARCH</TT> allows to check the results at this stage. Note
that for a two-dimensional spectrum, both options 1D and 2D can be
used (See <TT>HELP PLOT/SEARCH</TT>).

<P>
<LI>The command <TT>IDENTIFY/LONG</TT> allows an initial interactive 
identification, by wavelength, of some of the detected lines. Spectral
line atlas are provided in the instrument operating manuals.  The
command <TT>PLOT/IDENT</TT> visualizes the interactive identifications.

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<ADDRESS>
<I>Petra Nass</I>
<BR><I>1999-06-15</I>
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