TS ToupTek AE676 AstroEye USB3.0 Color Astronomy Camera with Sony IMX676 Sensor - D=10 mm, air-cooled
The AE676C is a versatile, high-performance astronomy camera designed to cover multiple astrophotography scenarios. Powered by the advanced Sony IMX676 sensor, it combines high infrared sensitivity, low read noise, and wide dynamic range to deliver outstanding results across planetary imaging, deep-sky photography, autoguiding, and all-sky monitoring.
Key Advantages: Sony IMX676 Color CMOS Sensor: 1/1.6" square sensor with 12.5 MP high resolution (3536x3536 pixels) Very high detail resolution: 2.0 µm pixel size Exceptional Infrared Sensitivity (High QE): Near-monochrome-level response in IR wavelengths 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 lensesWhat Can You Capture with AE676C?From planetary imaging and lunar details to deep-sky objects, meteors, Milky Way and all-sky monitoring, AE676C is a beginner-friendly multi-purpose astronomy camera designed for exploring different astrophotography possibilities.
Square Sensor for Flexible FramingAE676C 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 flexibilityAE676C 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.
Superior Infrared Sensitivity for Low-Light ImagingBuilt on Sony Starvis 2 technology, the AE 676C delivers exceptional sensitivity in both visible and infrared light. It has outstanding performance in low-light environments. With high QE at 825 nm and beyond, AE676C shows near full-pixel response comparable to monochrome sensors.
AR-Coated Protective Window for Maximum TransmissionAE676C 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 wavelengthsWhen 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 UseFeatures 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 Control: Precise (±0.1 °C) TEC cooling with PID control, down to 5 °C below ambient* - perfect for sharp, consistent long-focal-length imaging. Light Cooling Deep-Sky Camera Mode: Add the magnetic fan to boost cooling up to 20 °C below ambient*, reducing thermal noise during longer exposures in deep-sky imaging.*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 ROICapture 12-bit images natively, with software pixel binning from 1×1 to 8×8 for flexible output resolutions, and hardware binning from 1×1 to 2×2. Hardware ROI allows higher frame rates by reducing the readout area. It achieves up to 993 FPS at reduced resolution (8-bit mode). So AE676C is perfect for high-speed planetary imaging and solar and lunar detail capture.
Stable Performance with 512 MB DDR3 CacheEquipped with a 512 MB DDR3 buffer, AE676C 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 SwitchingThe AE676C 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 in bright targets while preserving highlights, ideal for bright targets. HDR Mode: Combines HCG low noise and LCG high full-well capacity for superior image quality.Flexible Mounting OptionsSupports 1.25" barrel, CS mount, C mount, M42M and M42F interfaces for different optical systems and imaging accessories.
Software CompatibilityConnect via StellaVita App, ToupSky software, or use ASCOM, INDI and DirectShow SDK. Third-party software compatible with these SDKs can also integrate via drivers available on the ToupTek Astro official website.
Drivers and SoftwareToupTek provides drivers and software for this camera, you can
download them from here.