Low-light imaging

Unprecedented image quality in low light conditions.

0.1 Lux sCMOS 0.1 Lux SPAD 512

Image quality limited only by fundamental physics​

Low-light imaging enables us to extract image features or objects even in extremely dark conditions. The ability to extract features or objects can be quantified by signal-to-noise ratio. The signal is equal to the amount of detected light, and maximized by the sensitivity or quantum efficiency. The noise is composed of shot noise (or Poissonian noise and defines the lowest possible noise) and other analog noise sources. The dominant analog noise source is readout noise. However, dark noise and column-amplification mismatches can also play a significant role in low-light imaging.

SPAD image sensors and camera eliminate analog noise sources by direct photon to digital transformation, limiting the signal-to-noise ratio only by the shot noise. This inevitable noise source in every particle based measurement is √N, with N being the number of detected photons. With the signal being N, the signal-to-noise ratio is thus √N.

Benefits of SPAD technology
for this application

Zero readout noise

Transforms light directly into a digital signal not altering its original (quantum) state.

Improved image quality

Clear, detailed images due to single photon detection and Poisson limited signal-to-noise ratio.

Examples / Application results

Satellite with a temporal resolution of 10 ms without dead time between frames. SPAD camera.

BOOTES1B telescope

Observe a GNSS satellite with a temporal resolution of 10 ms without dead time between frames. The satellite can be seen in the animation (middle-left).

SPAD 512 vs sCMOS

SPAD 512 vs sCMOS

This paper demonstrates the capabilities of our SPAD 512 camera in low light-conditions, and compares its SNR to a scientific CMOS camera. 

products

SPAD 512 vs qCMOS

Axiom Optics compares qCMOS and SPAD technologies under identical conditions, showing SPAD’s advantage in low-light and short-exposure conditions.

Recommended products

SPAD23 single-photon (photon-counting) detector array

SPAD 512

A complete camera with a 512×512 SPAD pixel array. The camera features fine gating circuitry to measure time-varying events, such as FLIM, and double FPGA read-out for the highest throughput. This camera is a perfect addition to any widefield microscopy system.

References

Pi Imaging support team

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