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. Author manuscript; available in PMC: 2010 Feb 12.
Published in final edited form as: J Mod Opt. 2007 Jan 1;54(2-3):239. doi: 10.1080/09500340600769067

Table 1.

Typical characteristics of different detectors used in single-molecule spectroscopy and imaging. QE: Quantum Efficiency; PC: Photocathode; ROS: Readout Stage. Except for the SPAD, the gain is expressed in counts per photo-electron, where “counts” is the number of electrons generated at the end of the photon conversion and photo-electron amplification processes. In other words, this is the number of electrons to be readout by the Analog-to-Digital Converter (ADC) of the detector. In a SPAD, millions of secondary charge carriers per avalanche can be generated, but they are all read as a single “count”

Detector Type QE @ 600
nm (%)
Gain
(cts/photon)
PC Dark
Count (d1)
(e/pixel/s)
ROS Dark
Count (d2)
(e/pixel/s)
Readout Noise
(e/pixel/s rms)
Excess
Noise
Factor
Model
CCD 95 1 0 0.002 5 @ 100 kHz
12 @ 2 MHz
1 PIXIS 512B, Roper
Scientific
ILT CCD 62 1 0 0.05 6 @ 10 MHz
8 @ 20 MHz
1 CoolSnap HQ,
Roper Scientific
ICCD Gen III 46 1,500 0.04 30 20 @ 1 MHz
32 @ 5 MHz
1.8 I-Pentamax, Roper
Scientific
EMCCD 92 1,000 0.5 0 45 @ 5 MHz
60 @ 10 MHz
1.4 Cascade 512B,
Roper Scientific
EBCCD/EBAPS 29 100 0.04 50 40 @ 54 MHz 1.1 NightVista E1100,
Intevac
Photon Counting 68 1 (106) 100 0 0 1 SPCM-AQR-14,
Perkin-Elmer

Excess noise factor value for maximum gain.

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