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ATR2600M Monochrome Cooled Astronomy Camera
Transitioning from One-Shot Color (OSC) to monochrome imaging is the defining upgrade for elite astrophotographers seeking uncompromising image quality. By eliminating the Bayer filter array, the ToupTek ATR2600M captures pure, unfiltered photons at every single pixel, unlocking the absolute maximum spatial resolution, contrast, and sensitivity of the acclaimed APS-C sensor format.
No Bayer Filter, Maximum Resolution: The Advanced Astrophotographer’s Choice
Transitioning from One-Shot Color (OSC) to monochrome imaging is the defining upgrade for elite astrophotographers seeking uncompromising image quality. By eliminating the Bayer filter array, the ToupTek ATR2600M captures pure, unfiltered photons at every single pixel, unlocking the absolute maximum spatial resolution, contrast, and sensitivity of the acclaimed APS-C sensor format.
True Pixel-Level Resolution
Without the artifacts and resolution loss of debayering interpolation, the native 6224 x 4168 matrix delivers unmatched structural definition and delicate astronomical details.
Sony IMX571 Back-Illuminated Sensor
Utilizing an APS-C optical format with an optimal 3.76μm pixel size, the sensor provides a generous 28.3mm diagonal imaging area designed to capture sweeping deep-sky vistas.
Peak Quantum Efficiency & Superior SNR
Capturing significantly more signal per pixel yields an inherently higher Signal-to-Noise Ratio (SNR), allowing you to pull faint nebula structures out of the dark background with exquisite delicacy.
Hardcore Hardware: 16-Bit ADC, >80% QE, and Zero Amp-Glow
Engineered for advanced and enthusiast deep-sky astrophotographers, the ATR2600M integrates benchmark hardware components. Every specification is optimized to deliver peak performance under rigorous comparison, offering an elite imaging platform that excels in data accuracy and sensor stability.
Native 16-bit ADC & 14 Stops of Dynamic Range
Achieves true 16-bit quantization for ultra-smooth grayscale transitions, preserving delicate star colors and preventing the cores of bright nebulae or galaxies from saturating.
Revolutionary High Full Well Mode
Offers a standard full well capacity of 51ke-, expandable up to an extraordinary 100ke- in High Full Well Mode to massively extend exposure flexibility and star dynamic range.
Ultra-Low Readout Noise
Features selectable high-gain and low-noise modes, dropping the readout noise to as low as 0.883e-, ensuring that the subtlest signals from distant deep-space objects are not lost in sensor noise.
Zero Amp-Glow Architecture
Meticulously engineered circuitry eliminates internal electroluminescence (amp-glow) entirely, guaranteeing immaculate, clean raw frames even during ultra-long exposures.
512MB DDR3 Ultra-Fast Buffer
An integrated 4Gb high-speed memory cache ensures stable, drop-free data transmission, effectively mitigating transfer errors over extended capture sequences.
Master Advanced Astrophotography with LRGB/SHO Filters in Urban Cities
The ATR2600M monochrome sensor serves as the ultimate engine for LRGB and SHO narrowband imaging. By isolating specific emission lines, this system pierces through city smog and artificial lighting to resolve authentic physical structures and rich nebula details from your backyard.
Unrivaled Narrowband Contrast
High quantum efficiency combined with zero internal amp-glow maximizes contrast, allowing you to capture high-exposure, razor-sharp narrowband frames even under heavy city light pollution.
Two-Stage Intelligent TEC Cooling
Features an integrated heat dissipation structure with a controllable electric fan that reduces the sensor temperature to 42℃ below ambient. Even during summer nights, it maintains a stable -5℃ to -10℃ all night long, allowing for seamless exposures up to 1 hour.
4-Level Adjustable Anti-Dew Technology
Adopts an advanced window heating element (consuming approx. 5W, fully controllable via software) to prevent dew condensation during high-humidity urban night sessions.
Professional Power Specification
Tailored for demanding setups, requiring a stable 12V 3A DC input (or 11−14V stable lithium battery source) to ensure reliable, high-load all-night duty cycles without frame corruption.
ATR2600M Performance Charts
HCG mode, HCG mode and high Full Well, LCG mode, LCG mode and high Full Well, and Spectral Response.
Mechanical Diagram
Cable Connection
Flexible Back Focus Connection
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