In astronomy, photometers are used to measure the brightness of stars or of other celestial objects. A photoelectric photometer records the electric current generated when light from a source falls onto a light-sensitive surface, kicking off electrons, which are then amplified into a measurable current by a photomultiplier. An area photometer, or imaging photometer, on the other hand, measures simultaneously the light intensity at each point of an extended object such as a nebula or galaxy using CCD detectors or an infrared array.
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