SWIR astronomy and research
400–1700 nm response supports visible-to-SWIR observation with the IMX992 InGaAs sensor.
Deep-sky cooled
ToupTek ATR992M is a SWIR InGaAs astronomy camera using the IMX992 sensor, with 5 MP (2560 × 2048), 3.45 µm pixels and 36 fps. Designed for swir astronomy and research, dust and haze penetration imaging, occultation and transient observation. Available from Precisometer for professional astronomy systems in the Benelux.

Applications & selection
400–1700 nm response supports visible-to-SWIR observation with the IMX992 InGaAs sensor.
Longer-wavelength response can reveal targets and structures that are difficult to distinguish in visible light alone.
Global-shutter capture and precise timing support synchronized observations of short astronomical events.
Suitable for scientific SWIR experiments, beam observation and quantitative imaging where a cooled camera is required.
Choose the ATR992M when your telescope and target benefit from 1/1.4-inch, 9.2 × 7.6 mm sensor coverage, 3.45 µm sampling, two-stage TEC, ΔT ≈30 °C and 400–1700 nm response.
Specifications
37 specification rows
The ATR992M is an astronomy camera in the ATR DSO cooled series, built around a Sony IMX992 SenSWIR InGaAs monochrome sensor sensor, 5 MP (2560 × 2048) resolution, 3.45 µm pixels, frame rates up to 36 fps, a USB 3.0 interface. It suits deep-sky cooled where reliable imaging performance and interface compatibility matter.
| Model | ATR992M |
|---|---|
| Status | Current |
| Application | Deep-sky cooled |
| Sensor | Sony IMX992 SenSWIR InGaAs monochrome sensor |
| Sensor Type | Global-shutter SWIR InGaAs monochrome CMOS |
| Sensor Size | 1/1.4-inch, 9.2 × 7.6 mm |
| Resolution | 5 MP (2560 × 2048) |
| Pixel Size | 3.45 µm |
| Shutter Type | Global shutter |
| Frame Rate | 36 fps |
|---|---|
| ADC | 12-bit |
| Peak QE | >90% |
| Dynamic Range | 8.5 stops |
| Read Noise | 68.34–80.16 e⁻ |
| Full Well | 70.3 ke⁻ |
| Spectral Range | 400–1700 nm |
| Interface | USB 3.0 |
|---|---|
| Mount | M42 / M54 astronomy adapters |
| Cooling | Two-stage TEC, ΔT ≈30 °C |
| Sensor Diagonal | 11.4mm |
|---|---|
| LCG Read Noise | 68.34-80.16e- |
| Maximum SNR | 44.9dB |
| Frame Buffer | 512MB |
| Sensor Chamber Window | Longpass protective window |
| Back Focal Distance | 17.5mm |
| Protective Window | Longpass |
| Color Filter Array | Mono |
| Exposure Time Range | 0.015 ms to 60 s |
| Gain Range | 1× to 150× |
| Supported Modes | Full resolution, hardware ROI, digital and hardware binning, HCG / LCG |
| Camera Mount | M42 × 0.75 female thread |
| Camera Dimensions | Diameter 80 mm × length 107.1 mm |
| Extra Ports | USB 2.0 hub × 1 for accessories; GPS port × 1 |
| Power Input | DC 12 V / 3 A, 5.5 × 2.1 mm connector |
| Supported OS | Windows XP / Vista / 7 / 8 / 10 / 11 (32 & 64 bit); macOS; Linux |
| SDK Support | Windows / Linux / macOS / Android SDK (C/C++, C#/VB.NET, Python, Java, DirectShow, Twain) |
| Software Compatibility | ToupSky; ASCOM platform; N.I.N.A; INDI; PHD Guiding; MaxIm DL; Nebulosity; SharpCap; FireCapture and more |
Technical media
Official sensor-response, performance, and mechanical imagery for the ATR992M.



Tell us your sensor, resolution, spectral range, frame-rate, interface, and software requirements and we will confirm the matching configuration and lead time.
The IMX992 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.
Compare the ATR992M with other ATR DSO cooled models and astronomy cameras in the range.
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