TS ToupTek AE676 AstroEye USB3.0 Monochrome Camera with Sony IMX676 Sensor - D=10 mm

TS ToupTek AE676 AstroEye USB3.0 Monochrome Astronomy Camera with Sony IMX676 Sensor - D=10 mm, air-cooled

The AE676M is a versatile, high-performance astronomy camera designed for a wide range of applications in astrophotography, including photography of planets, the Moon, the Sun, deep-sky objects, meteors, and the Milky Way.

Powered by the Sony IMX676 monochrome CMOS sensor, the AE676M combines full-spectrum sensitivity, Bayer-free pixel-level sharpness, NIR (Near-Infrared) penetration, and an ultra-compact design. Built to effortlessly master high-resolution solar/lunar mosaics, narrow-band deep-sky imaging, and NIR planetary photography.

Key Advantages:

Sony IMX676 monochrome CMOS Sensor: 1/1.6" square sensor with 12.5 MP high resolution (3536x3536 pixels)

Very high detail resolution: 2.0 µm pixel size

Full-Spectrum & Ultra-High NIR QE: Maintains 80%-88% high response at 800-850 nm.

Magnetic Detachable Cooling Fan Module: Switch between zero-vibration constant temperature mode and enhanced cooling mode

Built-in 512 MB DDR3 Cache: Stable data transfer with no frame drops, even under bandwidth limitations

Native 12-bit ADC + 16-bit HDR output: Preserves fine details and dynamic range, but also allows for faster capturing

HCG/LCG/HDR Gain Modes: Flexible optimization for different imaging targets

High Compatibility: Works with photography tripods, telescopes, guide scopes and wide-angle lenses

What Can You Capture with AE676M
From planetary imaging and lunar details to deep-sky objects, meteors, Milky Way, and all-sky monitoring, AE676M is a beginner-friendly multi-purpose astronomy camera designed for exploring endless astrophotography possibilities.

Square Sensor for Flexible Framing
AE676M features a 1/1.6" square sensor, eliminating the hassle of aligning different aspect ratios. It offers the benefits of:

Easier mosaic stitching without cropping

Faster post-processing workflow

Better framing flexibility

AE676M is especially well-suited for all-sky monitoring, meteor detection and Milky Way photography. The square format also pairs perfectly with fisheye and wide-angle lenses, maximizing image coverage.

Exceptional H-alpha & Near-Infrared Sensitivity
Powered by STARVIS 2 technology, the AE676M delivers over 95% relative response efficiency across the 600-750 nm range, maximizing the capture of H-alpha-rich targets, including solar prominences, flares, and emission nebula details.

Its outstanding sensitivity beyond 800 nm in the near-infrared spectrum enables stunning infrared Milky Way imaging through light pollution when paired with IR825/850 filters. Combined with narrowband filters, it provides efficient deep-sky signal acquisition even in light-polluted urban environments.

AR-Coated Protective Window for Maximum Transmission
AE676M features a dual-sided AR-coated optical window:

Reduces reflections and light loss

Protects against dust and physical damage

Enhances transmission across 400-1100 nm wavelengths

When paired with a long-pass filter starting at around 825 nm, such as the supplied ToupTek LP825, a TSIR850, the ASI850IRpass, or the Antlia IR850, it allows stunning infrared Milky Way imaging.

Modular Magnetic Cooling System for Flexible Use
Features a magnetic detachable rear cooling fan module for quick installation and removal. Single-stage TEC cooling combined with precision multi-channel heat dissipation supports long exposures while reducing thermal noise.

Fanless Constant Temperature Mode: PID temperature control algorithm enables precise cooling up to 5 °C below ambient. With ±0.1 °C stability and zero vibration, it´s ideal for long focal length telescopes requiring absolute sharpness.

With the magnetic fan attached, sensor temperatures drop by up to 20°C below ambient, greatly suppressing thermal noise during extended exposures and improving dark frame calibration.

*Tested under long-exposure conditions at 25 °C ambient temperature with proper ventilation. Actual performance may vary depending on environmental conditions and exposure duration.

Native 12-bit ADC & Hardware ROI
Capture 12-bit images natively with software binning from 1×1 to 8×8 and hardware binning from 1×1 to 2×2. Hardware ROI allows frame rates up to 993 FPS at reduced resolution (8-bit mode), making it perfect for high-speed planetary and solar/lunar detail capture.

Stable Performance with 512 MB DDR3 Cache
Equipped with a 512 MB DDR3 buffer, AE676M ensures stable data transfer and helps prevent frame drops even under bandwidth limitations. Read noise is as low as 1.01 e^- for clean backgrounds, while the 69.7 dB dynamic range preserves details in both bright and dark areas.

Seamless Multi-Mode Switching
The AE676M supports switching between HCG, LCG, and HDR modes, allowing independent selection according to different targets:

HCG Mode: Reduces readout noise while keeping high dynamic range for faint deep-sky object imaging and guiding.

LCG Mode: Prevents overexposure on bright targets while preserving highlights, ideal for bright targets.

HDR Mode: Combines HCG´s low noise with LCG´s high full-well capacity for maximum dynamic range (16-bit output).

Flexible Mounting Options
Supports 1.25" barrel, CS mount, C mount, M42M and M42F interfaces for different optical systems and imaging accessories.

Software Compatibility
Seamlessly connect via the StellaVita App, ToupSky software, or use ASCOM, INDI, and DirectShow SDKs for broad third-party software integration.

Drivers and Software
ToupTek provides drivers and software for this camera, you can download them from here.

- Camera body with adapter CS-mount-M42x0.75F
- Magnetic fan module
- M42x0.75F-M42x0.75F adapter ring (11 mm optical path)
- 1.25" extension tube
- CS-to-C adapter ring (5 mm optical path)
- CS-mount fisheye lens
- LP825 long pass filter cap
- USB3.0 high-speed cable, Type-A male to Type-C male (1.25 m)

Safety informations: PDF Download