There are two ways to describe the sensitivity of a camera. First, we can determine the minimum number of detectable photoelectrons. This can be termed the absolute sensitivity. Second, we can describe the number of photoelectrons necessary to change from one digital brightness level to the next, that is, to change one analog-to-digital unit (ADU). This can be termed the relative sensitivity.
The measurement of the sensitivity or gain can be performed in two distinct ways.
* If, following eq. , the input signal a can be precisely controlled by either "shutter" time or intensity (through neutral density filters), then the gain can be estimated by estimating the slope of the resulting straight-line curve. To translate this into the desired units, however, a standard source must be used that emits a known number of photons onto the camera sensor and the quantum efficiency () of the sensor must be known. The quantum efficiency refers to how many photoelectrons are produced--on the average--per photon at a given wavelength. In general 0 <= () <= 1.
* If, however, the limiting effect of the camera is only the photon (Poisson) noise (see Section 6.1), then an easy-to-implement, alternative technique is available to determine the sensitivity. Using equations , , and and after compensating for the offset (see Section 10.1), the sensitivity measured from an image c is given by:
where mc and sc are defined in equations and .
Measured data for five modern (1995) CCD camera configurations are given in Table 9.
Table 9: Sensitivity measurements. Note that a more sensitive camera has a lower value of S.
The extraordinary sensitivity of modern CCD cameras is clear from these data. In a scientific-grade CCD camera (C-1), only 8 photoelectrons (approximately 16 photons) separate two gray levels in the digital representation of the image. For a considerably less expensive video camera (C-5), only about 256 photoelectrons (approximately 512 photons) separate two gray levels.