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Deep-sky cooled

ATR585M

ToupTek ATR585M is a cooled deep-sky camera using the IMX585 sensor, with 8.3 MP (3840 × 2160), 2.9 µm pixels and 47 fps. Designed for deep-sky astrophotography, narrowband nebula imaging, high-resolution galaxy and lunar imaging. Available from Precisometer for professional astronomy systems.

Sensor
Sony IMX585 monochrome CMOS
Sensor Type
STARVIS 2 back-illuminated monochrome CMOS
Resolution
8.3 MP (3840 × 2160)
Pixel Size
2.9 µm
Frame Rate
47 fps
Interface
USB 3.0
ATR585M

Application context

Why this design is used

Choose the ATR585M when your telescope and target benefit from 1/1.2-inch, 11.2 × 6.3 mm sensor coverage, 2.9 µm sampling, two-stage TEC, ΔT ≥45 °C and 380–1100 nm response.

Deep-sky astrophotography

Two-stage TEC, ΔT ≥45 °C helps control thermal noise during long exposures of galaxies, nebulae and star clusters.

Narrowband nebula imaging

The monochrome IMX585 sensor is suited to H-alpha, O III and S II filter workflows.

High-resolution galaxy and lunar imaging

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

Photometry and time-series imaging

12-bit / 16-bit HDR acquisition, 88.6 dB HDR dynamic range and regulated cooling support repeatable quantitative observations.

Specifications

ATR585M

31 specification rows

The ATR585M is an astronomy camera in the ATR DSO cooled series, built around a Sony IMX585 monochrome CMOS sensor, 8.3 MP (3840 × 2160) resolution, 2.9 µm pixels, frame rates up to 47 fps, a USB 3.0 interface. It suits deep-sky cooled where reliable imaging performance and interface compatibility matter.

Sensor & Imaging

ModelATR585M
StatusCurrent
ApplicationDeep-sky cooled
SensorSony IMX585 monochrome CMOS
Sensor TypeSTARVIS 2 back-illuminated monochrome CMOS
Sensor Size1/1.2-inch, 11.2 × 6.3 mm
Resolution8.3 MP (3840 × 2160)
Pixel Size2.9 µm
Shutter TypeRolling shutter

Performance

Frame Rate47 fps
ADC12-bit / 16-bit HDR
Peak QE>91%
Dynamic Range88.6 dB HDR
Read Noise3.04–0.50 e⁻
Full Well38.9 ke⁻
Spectral Range380–1100 nm

Interface & Thermal

InterfaceUSB 3.0
MountM42 / M54 astronomy adapters
CoolingTwo-stage TEC, ΔT ≥45 °C

Additional Published Specifications

Legacy Model NameATR585M
Sensor Diagonal12.85mm
LCG Read Noise5.8-2.2e-
Maximum SNR46dB
Frame Buffer512MB
Sensor Chamber WindowAdjustable heating window
Back Focal Distance17.5mm/12.5mm
Protective WindowIR/AR
Color Filter ArrayRGGB
DDR3 Buffer512MB (4Gb)
Max ExposureUp to 3600 seconds (1 hour)
Power SupplyDC 12V / 3.3A

Technical media

Performance graphs and technical drawings

Official sensor-response, performance, and mechanical imagery for the ATR585M.

ATR585M quantum efficiency curve
ATR585M quantum efficiency curve
ATR585M HCG mode performance analysis
ATR585M HCG mode performance analysis
ATR585M dimensions and mount
ATR585M dimensions and mount

System integration

Integration and compatibility

Use these checks to connect ATR585M 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 IMX585 monochrome CMOS · Sensor Type: STARVIS 2 back-illuminated 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: 47 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: 88.6 dB HDR · Read Noise: 3.04–0.50 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 ATR585M

What lens mount is required for the ATR585M?

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 ATR585M use?

Sensor: Sony IMX585 monochrome CMOS · Sensor Type: STARVIS 2 back-illuminated 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 ATR585M connect to the acquisition computer?

Frame Rate: 47 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 ATR585M?

Dynamic Range: 88.6 dB HDR · Read Noise: 3.04–0.50 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.

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Model selection

Nearby series comparison

Compare ATR585M with the closest available models in the ATR DSO cooled family.

Selection parameterATR585M (current)ATR585CATR992M
SensorSony IMX585 monochrome CMOSSony IMX585 color CMOSSony IMX992 SenSWIR InGaAs monochrome sensor
Resolution8.3 MP (3840 × 2160)8.3 MP (3840 × 2160)5 MP (2560 × 2048)
Sensor size1/1.2-inch, 11.2 × 6.3 mm1/1.2-inch, 11.2 × 6.3 mm1/1.4-inch, 9.2 × 7.6 mm
Pixel size / frame rate2.9 µm2.9 µm3.45 µm

Other cameras on the IMX585 sensor

The IMX585 appears in 21 models across the catalogue, differing in cooling, shutter, interface and colour filter. Compare them side by side before settling on a variant.