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Deep-sky cooled

ATR294M

ToupTek ATR294M is a cooled deep-sky camera using the IMX492 sensor, with 11.6 MP (4128 × 2808), 4.63 µm pixels and 33 fps. Designed for deep-sky astrophotography, narrowband nebula imaging, high-resolution galaxy and lunar imaging. Available from Precisometer for professional astronomy systems.

Sensor
Sony IMX492 monochrome CMOS
Sensor Type
Back-illuminated 4/3-inch monochrome CMOS
Resolution
11.6 MP (4128 × 2808)
Pixel Size
4.63 µm
Frame Rate
33 fps
Interface
USB 3.0
ATR294M

Application context

Why this design is used

Choose the ATR294M when your telescope and target benefit from 4/3-inch, 19.11 × 13.0 mm sensor coverage, 4.63 µm sampling, two-stage TEC, ΔT ≥42 °C and 380–1100 nm response.

Deep-sky astrophotography

Two-stage TEC, ΔT ≥42 °C helps control thermal noise during long exposures of galaxies, nebulae and star clusters.

Narrowband nebula imaging

The monochrome IMX492 sensor is suited to H-alpha, O III and S II filter workflows.

High-resolution galaxy and lunar imaging

4.63 µm pixels balance image scale and detail for appropriately matched telescope focal lengths.

Photometry and time-series imaging

14-bit acquisition, 78.8 dB dynamic range and regulated cooling support repeatable quantitative observations.

Specifications

ATR294M

32 specification rows

The ATR294M is an astronomy camera in the ATR DSO cooled series, built around a Sony IMX492 monochrome CMOS sensor, 11.6 MP (4128 × 2808) resolution, 4.63 µm pixels, frame rates up to 33 fps, a USB 3.0 interface. It suits deep-sky cooled where reliable imaging performance and interface compatibility matter.

Sensor & Imaging

ModelATR294M
StatusCurrent
ApplicationDeep-sky cooled
SensorSony IMX492 monochrome CMOS
Sensor TypeBack-illuminated 4/3-inch monochrome CMOS
Sensor Size4/3-inch, 19.11 × 13.0 mm
Resolution11.6 MP (4128 × 2808)
Pixel Size4.63 µm
Shutter TypeRolling shutter

Performance

Frame Rate33 fps
ADC14-bit
Peak QE>80%
Dynamic Range78.8 dB
Read Noise7.53–1.42 e⁻
Full Well66 ke⁻
Spectral Range380–1100 nm

Interface & Thermal

InterfaceUSB 3.0
MountM42 / M54 astronomy adapters
CoolingTwo-stage TEC, ΔT ≥42 °C

Additional Published Specifications

Legacy Model NameATR3CMOS10300KMA
Sensor Diagonal23.1mm
LCG Read Noise7.53-6.42 e-
Maximum SNR48.2dB
Frame Buffer512MB
Sensor Chamber WindowAdjustable heating window
Back Focal Distance17.5mm/12.5mm
Protective WindowIR/AR
Color Filter ArrayRGGB
Gain ModesHCG (High Conversion Gain) / LCG (Low Conversion Gain)
DDR3 Buffer512MB
Max ExposureUp to 1 hour
Power SupplyDC 12V / 3A

Technical media

Performance graphs and technical drawings

Official sensor-response, performance, and mechanical imagery for the ATR294M.

ATR294M performance analysis HCG mode
ATR294M performance analysis HCG mode
ATR294M performance analysis LCG mode
ATR294M performance analysis LCG mode
ATR294M sensor optical format
ATR294M sensor optical format

System integration

Integration and compatibility

Use these checks to connect ATR294M to the surrounding optical, mechanical and control system. Every value shown is taken from this model's own specification record.

Lens and microscope interface
Mount: M42 / M54 astronomy adapters
Use a lens image circle that covers the sensor and check flange distance before adding C/CS, F-mount or M42 adapters.
Sensor and sampling
Sensor: Sony IMX492 monochrome CMOS · Sensor Type: Back-illuminated 4/3-inch monochrome CMOS
Match pixel pitch to the diffraction-limited spot the optics deliver. Sampling finer than the optics resolve multiplies data volume without adding information; sampling coarser discards resolution you have paid for.
Interface and data rate
Frame Rate: 33 fps · Interface: USB 3.0
Confirm the host can sustain the interface bandwidth continuously, not in burst. A camera that outruns the write path stalls acquisition rather than dropping quietly to a lower rate.
Cooling and noise floor
Dynamic Range: 78.8 dB · Read Noise: 7.53–1.42 e⁻
Judge these figures at the exposure time you will actually use. Cooling matters where dark current accumulates over seconds; read noise dominates short exposures where it never does.

Technical FAQ

Integration questions for ATR294M

What lens mount is required for the ATR294M?

Mount: M42 / M54 astronomy adapters. Use a lens image circle that covers the sensor and check flange distance before adding C/CS, F-mount or M42 adapters.

What sensor and pixel pitch does the ATR294M use?

Sensor: Sony IMX492 monochrome CMOS · Sensor Type: Back-illuminated 4/3-inch monochrome CMOS. Match pixel pitch to the diffraction-limited spot the optics deliver. Sampling finer than the optics resolve multiplies data volume without adding information; sampling coarser discards resolution you have paid for.

How does the ATR294M connect to the acquisition computer?

Frame Rate: 33 fps · Interface: USB 3.0. Confirm the host can sustain the interface bandwidth continuously, not in burst. A camera that outruns the write path stalls acquisition rather than dropping quietly to a lower rate.

What is the noise performance of the ATR294M?

Dynamic Range: 78.8 dB · Read Noise: 7.53–1.42 e⁻. Judge these figures at the exposure time you will actually use. Cooling matters where dark current accumulates over seconds; read noise dominates short exposures where it never does.

Need help choosing?

Tell us your sensor, resolution, spectral range, frame-rate, interface, and software requirements and we will confirm the matching configuration and lead time.

Open camera finder

Model selection

Nearby series comparison

Compare ATR294M with the closest available models in the ATR DSO cooled family.

Selection parameterATR294M (current)ATR294CATR428C
SensorSony IMX492 monochrome CMOSSony IMX294 color CMOSSony IMX428 color CMOS
Resolution11.6 MP (4128 × 2808)11.6 MP (4128 × 2808)7.04 MP (3200 × 2200)
Sensor size4/3-inch, 19.11 × 13.0 mm4/3-inch, 19.11 × 13.0 mm1-inch, 14.4 × 9.9 mm
Pixel size / frame rate4.63 µm4.63 µm4.5 µm

Other cameras on the IMX492 sensor

The IMX492 appears in 10 models across the catalogue, differing in cooling, shutter, interface and colour filter. Compare them side by side before settling on a variant.