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Editorial rank 20 of 99QHYCCD QHY268M
Full specificationAstronomy Camera
SensorSony IMX571 APS-C Mono CMOS
Resolution6280 x 4210 (26.1MP)
Pixel Size3.76 µm
CoolingTEC, up to -35°C below ambient
InterfaceUSB 3.0
4.6

QHYCCD

QHYCCD QHY268M

★★★★★ 4.6/5

The QHYCCD QHY268M is a superb monochrome astrophotography camera for serious deep-sky imagers, combining a large APS-C sensor, high QE, and strong cooling performance.

3.76µmpixel size4.6/5editor score5spec rows verified9in this category
  • Specification transcribed from manufacturer data
  • Scored against 8 peers in Cameras & imaging
  • Compromises listed in full below

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Verdict

The QHYCCD QHY268M is a superb monochrome astrophotography camera for serious deep-sky imagers, combining a large APS-C sensor, high QE, and strong cooling performance. While it demands investment in filters and computing resources, the image quality and flexibility make it a top-tier choice for advanced amateur and semi-professional astrophotography.

Key features

0126.1MP Sony IMX571 monochrome CMOS sensor
02Back-illuminated design for high quantum efficiency
03Dual-gain (HCG/LCG) readout modes
04Two-stage TEC cooling down to -35°C below ambient
05USB 3.0 high-speed data transfer
06Built-in mechanical shutter for automated darks/flats
0710-position filter wheel compatibility via QHY accessories

Full review

The QHYCCD QHY268M is a monochrome deep-sky imaging camera built around the Sony IMX571 APS-C format back-illuminated CMOS sensor, a chip prized among astrophotographers for its 16-bit readout, low read noise, and generous 26 megapixel resolution across a 3.76 micron pixel pitch. As a dedicated monochrome unit, it forgoes the Bayer color filter array found in its color sibling, the QHY268C, allowing every photosite to capture full luminance data without interpolation. This makes it especially suited to narrowband imaging with hydrogen-alpha, oxygen-III, and sulfur-II filters, as well as traditional LRGB workflows using a filter wheel, delivering sharper detail and better sensitivity than comparable color sensors when paired with the right filter set.

Thermal management is a central feature of the QHY268M, which incorporates a two-stage thermoelectric cooling system capable of pulling the sensor temperature down to roughly minus 35 degrees Celsius below ambient. This deep, regulated cooling suppresses dark current substantially, enabling long exposure subs with minimal thermal noise, a critical requirement for faint nebulae, galaxies, and other extended deep-sky targets that demand hours of cumulative integration time. The camera also offers dual gain modes, including a high-gain low-noise setting well suited to narrowband work under light-polluted skies, and a low-gain high-full-well setting favorable for broadband targets with a wide dynamic range, such as star clusters and galaxies with bright cores alongside faint outer structures. An anti-dew heating window further protects against condensation forming on the optical window during cold-weather sessions.

Physically, the QHY268M is built with a rugged, compact housing designed for observatory and field use, featuring a standard M54 or M42 nosepiece thread depending on configuration, along with USB 3.0 connectivity for fast data transfer during high-frame-rate or large-file deep-sky sessions. It integrates smoothly with popular imaging software such as N.I.N.A., SharpCap, and MaxIm DL through native SDK and ASCOM driver support, making it a flexible choice for both automated observatory setups and portable rigs used by amateur astronomers. Combined with its low amp-glow design and mechanical shutter-free readout, the QHY268M has become a favored tool among astrophotographers seeking a high-resolution, scientifically capable monochrome sensor for capturing detailed, high-fidelity images of the night sky.

The trade-off

What you gain, what you give up

6 strengths · 5 compromises

Strengths

  • Excellent quantum efficiency (~91% peak) for faint targets
  • Very low read noise in HCG mode
  • Effective cooling minimizes thermal noise on long exposures
  • Large APS-C sized sensor with wide field coverage
  • Robust build quality with metal housing
  • Mono sensor allows narrowband imaging flexibility with filters

Compromises

  • Expensive compared to entry-level astro cameras
  • Requires separate filter wheel purchase for LRGB/narrowband
  • Large file sizes demand fast storage and good PC specs
  • Learning curve for gain/offset optimization
  • Bulky form factor adds weight to imaging train

Nearby

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