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.
|