
ZWO ASI2600MM Pro USB 3.0 Cooled Monochrome Astronomy Imaging Camera
Manufacturer Part # ZWO ASI2600MM-P
Manufacturer Part # ZWO ASI2600MM-P
For astrophotographers looking to capture deep-sky objects with exceptional detail, dynamic range, and noise control, the ZWO ASI2600MM Pro is a top-tier monochrome camera that combines cutting-edge CMOS technology with advanced cooling and high efficiency. With its large APS-C sensor, zero amp glow design, and remarkable quantum efficiency, this camera is a superb choice for capturing galaxies, nebulae, and star clusters with clarity that rivals professional observatory systems.
At the core of the ASI2600MM Pro is the Sony IMX571 back-illuminated CMOS sensor, an APS-C format chip with a high resolution of 26 megapixels. The sensor has a total pixel array of 6248 x 4176, giving astrophotographers an expansive field of view while maintaining fine image detail. The large sensor size makes it well-suited for deep-sky imaging, as it can frame substantial portions of the night sky in a single exposure, reducing the need for mosaics when capturing wide targets such as the Andromeda Galaxy or the Orion Nebula.
Unlike smaller sensors that may limit the field of view or require heavy cropping, the APS-C format of this camera allows for more natural compositions and better framing of celestial objects. The pixel size of 3.76 microns strikes an ideal balance between resolution and sensitivity, delivering sharp images while retaining strong signal-gathering capability.
A crucial aspect of any astrophotography camera is its ability to collect and process light efficiently. The ASI2600MM Pro offers an outstanding peak quantum efficiency of 91%, meaning a greater portion of incoming photons are converted into useful signal rather than being lost to sensor inefficiencies. This high quantum efficiency is particularly beneficial for deep-sky imaging in narrowband, where every bit of captured light is essential for bringing out faint structures in nebulae and galaxies.
The camera also features an impressive full well capacity of 50,000 electrons per pixel, which reduces the risk of bright stars oversaturating and washing out detail in surrounding objects. The deep well depth contributes to the camera's ability to achieve a 14-stop dynamic range, ensuring that both the brightest and faintest structures within an image are preserved with excellent contrast.
One of the most significant challenges in long-exposure imaging is dealing with amp glow, an artifact that appears as an unwanted gradient in many CMOS sensors when exposed for extended periods. The ASI2600MM Pro is designed with zero amp glow technology, meaning there are no artificial light patterns interfering with dark backgrounds or fine details in deep-sky objects. This feature simplifies post-processing, eliminating the need for complex amp glow corrections in calibration frames.
In addition to zero amp glow, the camera excels in noise control. The read noise is as low as 0.7 electrons at high gain settings, significantly reducing unwanted graininess in images. This is particularly important when stacking multiple exposures, as lower noise levels help preserve fine structures without excessive smoothing or detail loss.
Thermal noise can be a major challenge for deep-sky imaging, especially during long exposures where heat-generated noise can accumulate over time. The ASI2600MM Pro features a built-in two-stage TEC (thermoelectric cooling) system, which can cool the sensor up to 35 to 40 degrees Celsius below ambient temperature. By keeping the sensor consistently cool, the camera minimizes thermal noise, resulting in cleaner images with reduced need for dark frame calibration.
The cooling system operates efficiently with a 12V DC power source, making it suitable for both permanent observatory setups and portable imaging rigs. Additionally, the sensor chamber is sealed to prevent internal condensation, ensuring reliable performance in a variety of environmental conditions.
Unlike many CMOS cameras that operate with 12 or 14-bit analog-to-digital conversion, the ASI2600MM Pro features a true 16-bit ADC. This results in significantly smoother gradations between light and dark regions, preserving delicate details in nebulosity, galaxy arms, and fine star structures.
A 16-bit ADC translates to a 65,536-level grayscale depth per pixel, compared to just 4,096 levels in a 12-bit camera. This improvement is crucial for capturing subtle variations in brightness, ensuring that extended dynamic range targets, such as the bright core and faint outer halo of a galaxy, are rendered with natural and accurate contrast.
The camera includes an HCG (High Conversion Gain) mode, which allows astrophotographers to optimize the balance between read noise and dynamic range depending on their imaging conditions. At higher gain settings, the read noise drops dramatically without sacrificing full well capacity, making the camera an excellent choice for both short and long-exposure imaging.
Data transfer is handled through a fast USB 3.0 interface, ensuring quick frame downloads with minimal lag. A built-in 256MB DDR3 memory buffer further stabilizes image capture, reducing frame dropouts and enhancing performance when capturing long imaging sequences.
As a monochrome camera, the ASI2600MM Pro is specifically designed for use with LRGB and narrowband filters, offering maximum flexibility in astrophotography. Monochrome sensors capture significantly more detail compared to color sensors because they dedicate 100% of their pixels to light collection without interpolation.
When paired with a high-quality electronic filter wheel, the ASI2600MM Pro can produce stunning full-color astrophotography images with better contrast and resolution than one-shot color cameras. It is also highly effective for narrowband imaging, allowing astrophotographers to capture deep-sky objects with superior signal-to-noise ratio, even under light-polluted skies.
Despite its powerful performance, the ASI2600MM Pro remains highly portable. The camera body weighs approximately 1.54 pounds (24.7 ounces), making it a lightweight option for telescope setups of all sizes. Whether mounted on a compact refractor for wide-field imaging or paired with a large reflector for deep-space work, the camera’s weight and size ensure compatibility with a wide range of astrophotography rigs.
Its power efficiency is also a key advantage, with a power draw of only 3A at full cooling. This makes it an excellent choice for field astrophotographers running off portable power stations, as well as those with observatory setups looking to minimize power consumption.
With its combination of high resolution, excellent dynamic range, and cutting-edge cooling technology, the ZWO ASI2600MM Pro is one of the best monochrome astrophotography cameras available. Whether you are capturing deep-sky nebulae, distant galaxies, or fine star structures, this camera provides professional-grade performance for amateur and advanced astrophotographers alike.
Please note that the camera needs to be connected to an external 11-15v power supply to implement the cooling function. We recommend you use 12V@3A DC adapter (5.5*2.1mm, center pole positive) or lithium battery with 11-15V to power the camera.
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ZWO has all their information available for download on their website in a perfectly laid out section. Check it out here for software and drivers and here for manuals and guides.
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Sensor | Back-Illuminated CMOS |
ADC | 16 bit |
Back Focus | 17.5 mm |
Color or Mono | Mono |
Cooled or Uncooled | Cooled |
Dynamic Range | 13.9 stops |
Full Resolution Frame Rate | 3.51fps |
Full Well | 50ke |
Mega Pixels | 26.1 mp |
Peak QE | 80% |
Pixel Array | 6248 x 4176 |
Pixel Size | 3.76 microns |
Read Noise | 3.3e |
Sensor Diagonal | 28.3 mm |
Sensor Type | CMOS |
Sensor | Sony IMX571 CMOS |
Guide Port | N/A |
WIndow | AR |
Exposure Range | 32us - 2000s |
Weight | 1.5 pounds |
Normal Num Pixel High | 4176 |
---|---|
Normal Num Pixel Wide | 6248 |
Pixel Array | 26.1 mega pixels |
Pixel Size | 3.76 |
Weight | 1.5 pounds |
Warranty | 2 years |
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