ATR585M features a Sony IMX585 back-illuminated mono sensor with 3840×2160 resolution and 2.9μm square pixels. The camera is designed specifically for astrophotography with ultra-low readout noise (0.50e⁻), zero amp-glow, two-stage TEC cooling system (up to 45°C below ambient), 512MB DDR3 buffer, built-in 12-bit ADC, 38.9ke full well, and supports high frame rate mode (24 fps@12-bit / 47 fps@8-bit RAW).
ATR585M features the Sony IMX585 back-illuminated mono sensor with 1/1.2-inch optical format, ideal for high-sensitivity deep sky photography with exceptional quantum efficiency and ultra-low noise.
The Sony IMX585 sensor features exceptional quantum efficiency above 91% peak, with excellent response across the visible and near-infrared spectrum, making it ideal for narrowband and broadband deep sky imaging.
ATR585M camera has a 512MB (4Gb) ultra-fast DDR3 memory buffer to ensure stable image transmission, easing the burden on your computer's transmission system and effectively reducing amp-glow.
ATR585M has been carefully designed and is able to achieve zero amp-glow photo shooting. The comparison below shows different cameras at 20°C with 5-minute exposure time. ATR585M demonstrates zero amp-glow performance.
With Amp-glow
ATR585M: Zero Amp-glow
ATR585M features a two-stage Thermoelectric Cooling (TEC) with controllable fan, allowing the sensor to operate at temperatures up to 45°C below ambient under long exposure. The exposure time can be set for up to 1 hour, ensuring every detail is captured with minimal dark current.
The integrated heat dissipation structure and efficient cooling module ensure stable operation. The PID algorithm allows TEC to be precisely regulated towards the target temperature with ±0.1°C deviation, maintaining stable cooling throughout the night.
ATR585M adopts advanced anti-dew technology with a heating function consuming about 5 watts (can be turned off via software). The dew heater at the protection window has 4 adjustable levels.
High Conversion Gain (HCG) Mode: Optimized for ultra-low read noise (0.50e⁻ to 0.79e⁻), ideal for deep sky long exposure imaging where read noise is critical.
Low Conversion Gain (LCG) Mode: Optimized for higher full well capacity (38.9ke⁻), providing wider dynamic range for bright objects and shorter exposures.
HDR Mode: Combines HCG and LCG for extended dynamic range (88.6 dB), perfect for capturing both faint nebulae and bright stars in a single image.
| Sensor | Sony IMX585 Back-Illuminated Mono CMOS |
|---|---|
| Resolution | 3840 × 2160 (8.3MP) |
| Pixel Size | 2.9μm × 2.9μm |
| Optical Format | 1/1.2-inch (diagonal 12.85mm) |
| ADC | 12-bit (16-bit @ HDR) |
| Full Well | 38.9 ke⁻ (LCG mode) |
| Read Noise | 0.50e⁻ to 3.04e⁻ |
| QE Peak | >91% |
| Frame Rate | 24 fps @ 12-bit / 47 fps @ 8-bit (USB 3.0) |
| DDR3 Buffer | 512MB (4Gb) |
| Cooling | Two-stage TEC, up to 45°C below ambient (long exposure) |
| Max Exposure | Up to 3600 seconds (1 hour) |
| Power Supply | DC 12V / 3.3A |
| Interface | USB 3.0 / USB 2.0 |
| Shutter Type | Rolling shutter |
| Protection Window | AR-window (mono) |
ATR585M can be connected to a telescope with proper adapter (M42M-1.25" or M42M-2") or camera lens (Nikon F-M42 or EOS EF-M42 adapter). The female flange to sensor is 17.5mm.
Important: ATR585M requires external DC 12V/3A power supply. USB 3.0/2.0 is used only for data communication. The USB-HUB allows connection with other devices (filter wheel, guiding camera, etc.).
Get exclusive expert reviews, new launches, and crucial updates sent directly to you.