
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.
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Buy the AE676M and leave an honest review on this product page (including text + at least 2 photos of your astrophotography shots or setup/unboxing) to unlock double rewards:
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8% OFF Coupon: Get an 8% discount code for your next purchase (cannot be combined with other discounts). Valid through October 31.
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Why Sony IMX676 Square Sensor? Framing Perfected, Effortless Mosaics.

- Seamless Mosaic Stitching: Perfect symmetry reduces overlap waste and removes tedious cropping when assembling high-resolution solar and lunar panoramas.
- 360° All-Sky & Wide-Field Coverage: Pairs seamlessly with fisheye and short-focal-length lenses for round field-of-view targets, meteor tracking, and all-sky monitoring without wasting active sensor area.
- Rotation-Free Target Framing: Center emission nebulae, globular clusters, or planetary disks effortlessly without constantly re-rotating your camera train.
- Faster Post-Processing Workflow: Standardized 1:1 square frames simplify stacking, alignment, and channel combination across LRGB and narrowband workflows.
What Can You Capture with AE676M
Designed to cover a wide range of multi-role imaging needs, the AE676M features a 1/1.6” square mono sensor, giving imagers the flexibility to capture solar, lunar, planetary, and deep-sky targets with a single camera. From high-resolution lunar mosaics to near-infrared planetary details and narrowband DSO imaging, AE676M combines full-spectrum sensitivity, ultra-high NIR quantum efficiency, low read noise, and high-speed framing for consistently crisp, detailed results.
Why Choose the AE676M

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.

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.











