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AE676M

Name: AE676M
Brand: ToupTek Astro
Price: 409.0 USD
Availability: InStock

AstroEye Multi-purpose Astronomy Camera

$409.00 USD

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Description

REVIEWS

AE676M Multi-purpose Astronomy Camera

Capture Planets, Moon, Sun, Deep Sky, Meteors & Milky Way with One Multi-purpose Astronomy Camera.

Powered by the Sony IMX676 mono 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.

📷 Sony IMX676 Mono CMOS Sensor: 1/1.6” square sensor with 12.5MP high resolution.

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

❄️ Magnetic Detachable Cooling Fan: Switch between zero-vibration mode & enhanced cooling.

⚡ Built-in 512MB DDR3 Cache: High-speed, stable data transfer without frame drops.

📊 Native 12-bit ADC + 16-bit HDR: Preserves fine details and dynamic range.

🎛️ HCG / LCG / HDR Gain Modes: Flexible optimization for any imaging scenario.

🔭 High System Compatibility: Works with tripods, telescopes, guide scopes, and wide-angle lenses.

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

The AE676M features a 1/1.6" square sensor, eliminating the hassle of aligning different aspect ratios:

Easier mosaic stitching without tedious cropping
Faster post-processing workflow
Better framing flexibility for diverse targets

Especially well-suited for all-sky monitoring, meteor detection, and Milky Way photography. The square format pairs perfectly with fisheye and wide-angle lenses to maximize optical coverage.

Exceptional H-alpha & Near-Infrared Sensitivity

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

Its outstanding sensitivity beyond 800nm 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.

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.

Light Cooling Deep-Sky Mode

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 based on environment.

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.

Equipped with a 512MB DDR3 buffer, the AE676M ensures ultra-low readout noise (as low as 1.01 e⁻) and a high dynamic range of 69.7dB without frame drops, preserving details in both highlights and shadows.