Scientific Cameras
Quantitative cutting-edge cameras for scientific research, engineered with precision and innovation, and offering comprehensive solutions for researchers across a wide range of new and emerging applications. Our detectors offer everything from high sensitivity for low-light single-molecule imaging to high-speed for capturing dynamic events across large fields of view, resulting in unmatched performance and reliability.
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Kinetix
High Speed, Large Sensor sCMOS
- Faster: 500 fps full-frame to capture dynamic samples
- Bigger: 29 mm, 10 MP sensor for high-content imaging
- More Sensitive: 96% QE and sub-electron read noise
COSMOS
Large Format, Low-Noise Astronomy Cameras
- Large 81 x 81 mm sensor size
- Up to 20 fps full frame
- Deeply cooled, low noise sensor
Pylon IR
Low-Noise, Deep Cooled, InGaAs Spectroscopy Camera
- Cryogenically cooled InGaAs detector with fast spectral rate and lowest system read noise
- Integrated cold sheet reducing ambient noise
- Up to 6600 spectra/s
BLAZE
Award Winning Cameras for Spectroscopy
- Up to 300% higher NIR sensitivity
- True -100°C cooling
- Permanent vacuum guarantee
Evolve
High Sensitivity EMCCD
- Highly sensitive EMCCD for science
- 13 or 16 µm pixel size options
- High-speed readout
INFINITY Series
High Performance Microscope Cameras
- Up to 20 MP in resolution
- Scientific in-camera glass for consistent quality
- Feature-rich INFINITY ANALYZE software package
Iris
High Resolution, Large FOV Imaging
- High resolution imaging even at low magnifications
- Small 4.25 µm pixels across huge arrays
- Up to 25 mm field of view
KURO
Back-Illuminated CMOS
- Back-illuminated CMOS 95% QE
- High UV Sensitivity
- 1.3 e⁻ read noise (RMS)
LANSIS
The Latest in CCD Array Detector Technology
- High performance AIMO CCD sensor, Grade 1
- Highest average QE from UV to NIR
- Back-illuminated deep-depletion CCD
Moment
Ultra-Compact High Speed CMOS
- Ultra-compact CMOS for science
- Low Noise, High Speed Imaging
- True Global Shutter
NIRvana
For low-light NIR and SWIR imaging and spectroscopy
- Designed for both end-user and OEM integration
- Ultra-low cooled cameras
- High sensitivity
PI-MAX 4
Ultrafast, Intensified Cameras
- Ultrashort ≤500 ps gating
- Fast 1 MHz gate opening rate
- Built-in precision timing and delay generator
PIXIS
High-Performance, Low-Noise CCD Cameras
- Broad range 120–1100 nm
- Lifetime vacuum guarantee
- Low dark current
Prime 95B
Back-Illuminated sCMOS with Large Pixels
- Highly sensitive back-illuminated sCMOS for science
- 95% QE and low noise levels
- Large 11 µm pixels
Prime BSI
Back-Illuminated sCMOS with Low Read Noise
- Highly sensitive back-illuminated sCMOS for science
- 95% QE and ultra-low 1.0 e⁻ read noise
- Balanced 6.5 µm pixels
Prime BSI Express
Compact, Powerful sCMOS for High-Speed Imaging
- Highly sensitive back-illuminated sCMOS for science
- 95% QE and ultra-low 1.0 e⁻ read noise
- 95 fps over USB 3.2
ProEM
Ultralow Light Detection Camera
- Deep cooling
- ≥95% quantum efficiency
- eXcelon 3 technology
PyLoN
Extremely Low Noise Liquid Nitrogen Cooled Cameras
- -120 °C cryogenic cooling
- 1800 spectra per second
- Ultra low noise
Retiga CCD Family
- Low Noise, High Sensitivity CCDs for science
- Fast and Flexible Microscope Cameras
- Designed for specific applications
Retiga E
Cooled, Low-Noise CMOS For Integration
- Long Exposure CMOS (over 60 minutes)
- Cooled and Low-Noise
- Compact and Easy Integration
SOPHIA
Ultra-Low-Noise CCD Cameras
- Ultra-low-noise electronics with 95% QE
- All-metal hermetically sealed vacuum design
- Engineered for dark calibration and exposure control