Figure 2.3 shows the relative sizes of the PHT-P
and -S apertures, and the PHT-C detector pixels. They were centred in
the specified unvignetted field of view of
inside the
field of view of the ISO telescope.
Note that the gaps between the individual PHT-C detector pixels are
real. These gaps may have influenced the choice of the observing mode,
in particular, if the flux of a source or its spatial flux
distribution had to be measured accurately.
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