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For certain types of experiment, it may be important to note that    the IPCS
is a much larger detector than any of the CCDs currently    available on the
INT. For spectroscopic observations, the INT IPCS    provides 2044 pixels along
the dispersion direction, each    about 15 
m in size. The GEC CCD   
provides 578 pixels along the dispersion direction, each 22
m    in size.
This means that for a fixed wavelength resolution,    the IPCS provides almost
2.5 times the wavelength coverage.    The usefulness of this multiplex
advantage depends very much    on the type of experiment being performed. For
an experiment    where wavelength coverage is important, it might mean that   
the IPCS is the preferred detector, even though the integration    time to
reach the desired signal to noise ratio in    each resolution element is 2-3
times longer. A new generation of CCDs    with 
 to 
 pixels is
becoming available for astronomical observations and we hope to offer it on the
INT from 1990.