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

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<H1><A NAME="SECTION003110000000000000000">
Introduction</A>
</H1>
The purpose of this chapter is to describe the Optopus package, the 
set of programs, now implemented in MIDAS, which helps the Optopus
observers to prepare their observations in a fast and easy way.

<P>
The Optopus facility is designed to enable conventional use of the
Boller and Chivens spectrograph to be extended to perform
spectroscopy of multiple or large extended objects simultaneously 
(see G. Lund, 1986,<I>OPTOPUS, ESO Operating Manual No. 6</I>, for 
further details).  At present, Optopus is available for use at 
the 3.6m telescope only.

<P>
The fibre component of Optopus consists of 54 separately cabled
optical fibres which enable light to be guided from freely distributed
points in the focal plane at the entrance slit of the spectograph. The
fibre ends are precisely located at the telescope focal plane by means
of accurately drilled templates, known as ``starplates''.

<P>
The Optopus starplates (one for each observed field) are prepared in
an automatic process in the ESO workshop on La Silla, after the observer 
has produced a drilling instruction file from his/her coordinate dat for each
field. The Optopus package in MIDAS enables Optopus
observers to create the file with the instuctions for the
computer-controlled milling machine. It has been designed to be as
``user friendly'' as possible. All the commands request a minimum
amount of input from the user; in addition they verify use of
correct parameters.

<P>
Please do not forget that the instruction file has to be transferred
to La Silla. Also, note that the milling machine on the mountain can
only produce 2 to 3 starplates per day. If in doubt, always check with
the Visiting Astronomers Section at ESO Headquarters in Garching at
least three months prior to the observations.

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