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In order to image a nonzero field of view, the collimator
has to accept off-axis beams, and be physically wider than
. Figure 3 shows the path of off-axis
beams through the optical system.
For the simplified case in which
the off-axis beams are parallel to the optical
axis (``telecentric'') and we have abstracted the collimator
as a simple lens, then
[Side note: For a complex lens, the
isn't necessarily the diameter
of all of the collimator glass, but the diameter of the
collimator entrance pupil. The entrance pupil of a lens by itself
is not the same thing as the pupil of the whole system,
indicated by the vertical dotted line. In both cases, pupil means
the image of an aperture stop, but for the whole system, the aperture
stop is the primary mirror.]
Note that the collimator must have total f-number
The whole collimator lens is faster than the beam delivered by the telescope, because it has to be wide enough to accept the off-axis beams. Faster lenses or mirrors that accept light from larger off-axis angles are harder to construct. Imaging over a wide field also has to contend with the curvature of the telescope focal plane. In practice, both the size of the available detector and the requirement of good image quality for off-axis points set limits on the field of view of an instrument.