As mentioned above, CCD chips have a wide dynamic range within which
their response is essentially linear. However, if the illuminating
light is sufficiently bright the response will become non-linear and will
ultimately saturate (that is, an increase in the intensity of the
illumination produces no change in the recorded signal). In principle
the response in the non-linear region can be calibrated. However, in
practice, the onset of saturation is sufficiently rapid that it is more
sensible to limit exposures to the linear region. In order to prevent
saturation it is usual to a take a series of short exposures rather than
a single long exposure of equivalent duration. The individual short
exposures can then simply be added during the data reduction. This
technique offers other advantages, for example in the detection and removal
of cosmic-ray events (see below). Usually the documentation for the
instrumentation that you are using will include the range of intensities
over which the response is linear.
The 2-D CCD Data Reduction Cookbook