Aries 6504 Pro

Single-Photon-Level sCMOS Camera

  • 0.43 e- (RMS) readout noise
  • 297 fps @ 4.2 MP
  • 0.01 e⁻/p/s @ −20 °C
  • 95% QE,@ 450nm
  • 6.5 μm pixel size
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Overview

The Aries 6504 Pro is built on a next-generation back-illuminated sCMOS platform, delivering substantial improvements in readout noise, frame rate, and dark current. In high-sensitivity readout mode, it achieves 0.43 e⁻ (RMS) readout noise for single-photon-level signal discrimination, complemented by 297 fps at 4.2 MP in high-speed readout mode and a dark current of ≤0.01 e⁻/pixel/s @ −20 °C. Together, these capabilities extend the performance envelope of sCMOS cameras for demanding low-light and high-speed imaging applications.

  • 95% QE & 0.43e-(RMS)
    Single-Photon-Level Resolution

    The Aries 6504 Pro is optimized on a back-illuminated sCMOS platform with 95% QE and 6.5 μm pixels. In high-sensitivity readout mode, it achieves 0.43 e⁻ (RMS) readout noise with 99 fps at 4.2 MP. Photon probability density fitting over 100,000 frames shows distinguishable photon distributions, supporting quantitative and stable measurements at extremely low photon levels.

    95% QE & 0.43e-(RMS) <br>Single-Photon-Level Resolution
  • 297 fps @ 4.2 MP
    High-Speed with Sub-Electron Noise

    In high-speed mode, the Aries 6504 Pro operates at up to 297 fps at full 4.2 MP resolution, representing a threefold increase in frame rate compared with previous-generation sCMOS cameras of the same sensor format. Sub-electron readout noise down to 0.8 e⁻ is maintained at full resolution, enabling efficient photon utilization in high-speed, low-light conditions.

    297 fps @ 4.2 MP<br> High-Speed with Sub-Electron Noise
  • 170 fps @ 16bit
    High Speed & High Dynamic Range

    The high dynamic range mode supports 170 fps at 4.2 MP, combined with a full well capacity of up to 15 ke⁻ and true 16-bit digitization. This allows accurate capture of both low- and high-intensity signals within the same acquisition, supporting quantitative imaging across a wide dynamic range.

    170 fps @ 16bit<br>  High Speed & High Dynamic Range
  • 0.01 e-/pixel/s @ −20 °C
    Low Dark Current for Long-Exposure

    At −20 °C, the Aries 6504 Pro exhibits a dark current as low as 0.01 e⁻/pixel/s, approximately one-fifth that of previous-generation 6.5 μm sCMOS cameras. This reduction significantly improves long-exposure performance and supports applications requiring extended integration times under low-light conditions.

    0.01 e-/pixel/s @ −20 °C<br>  Low Dark Current for Long-Exposure

Specification >

  • Model: Aries 6504 Pro
  • Sensor Type: BSI sCMOS
  • Sensor Model: GSENSE6504BSI
  • Peak QE: 95 % @ 450 nm
  • Color/Mono: Mono
  • Array Diagonal : 18.8 mm
  • Effective Area: 13.3 mm x 13.3 mm
  • Resolution: 2048 (H) x 2048 (V)
  • Pixel Size: 6.5 μm x 6.5 μm
  • Full-Well Capacity: 15ke- @ HDR
  • Dynamic Range: 91dB @ Sensitive
  • Frame Rate: 99fps @ Sensitive mode

    170fps @ HDR mode

    297fps @ Speed mode
  • Readout Noise: 0.43e-(RMS) @ Sensitive mode
  • Shutter Type: Rolling, Global reset
  • DSNU: 0.2 e-
  • PRNU: 0.3 %
  • Cooling Method: Air, Liquid
  • Max. Cooling Temperature: Liquid:-20℃ @ Liquid temperature 20℃

    Air:-10℃ @ Ambient temperature 25℃
  • Dark Current: 0.01 e-/pixel/s @-10℃
  • Binning: 2 x 2, 4 x 4
  • ROI: Support
  • Trigger Mode: Hardware, Software
  • Output Trigger Signals: Readout End,Global Exposure,Exposure Start, Trigger Ready,first row,any row,High,Low
  • Trigger Interface: SMA x 4
  • Data Interface: USB3.2 Gen2, CXP2.0 x 2
  • Data Bit Depth: 12 bit, 16 bit
  • Optical Interface: C-mount
  • Power Supply: 12 V / 8 A
  • Power Consumption: 45 W
  • Dimensions: 85 mm x 85 mm x 127 mm *
  • Weight: 995 g
  • Software: Mosaic, SamplePro
  • SDK: C, C++
  • Operating System: Windows, Linux
  • Operating Environment: Windows 10/11、Ubuntu 22.04
  • * Remark:: The dimensions listed refer to the bare camera body only; water-cooling connectors, adapters, and interfaces are not included. For full details, see the mechanical drawing.
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