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<H1><A NAME="SECTION003760000000000000000">
Order extraction</A>
</H1>

<P>
After background subtraction, the spectral orders can be
extracted. This is done by defining offsets in x-direction (with
respect to the center of both fibers) and summing up the flux within a
defined slit-width around these offsets. Both fibers are treated
completely separately.

<P>
For reason of efficiency and simplicity, this is done in two
steps. 

<P>
<UL>
<LI>
First, the pixels are re-ordered (rectified) in a new 2-D frame. It
is important to note that this step involves <EM>no</EM> resampling.  The
fractional pixel offsets are kept in a separate file. The
corresponding command is RECTIFY/FEROS.
<LI>
Second, the fluxes are summed up, producing a new 2-D frame
(pixel-order space) for each fiber. The corresponding command is
EXTRACT/FEROS.
</UL>
<P>
The extraction can be done by straight summation or by using an
optimum extraction algorithm which also detects and removes cosmic ray
events. Optimum extraction requires a good knowledge of the
cross-order profile (COP). For FEROS, this profile is - due to the
image slicer - very complicated. It is approximated by fitting the
fractional flux per pixel at several distances from the center of the
COP as a function of position along the order with a polynomial. Since
rebinning has to be avoided, this step is complex and CPU
intensive. Thus, the COP can be saved for further use.  For FEROS, the
COP is typically determined from a flat-field exposure and later used
for extraction of object spectra. This assumes that the COP does not
change its profile, which can reasonably be assumed only for fiber-linked
spectrographs.

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