The ASI2600MM Pro uses Sony’s latest back-illuminated IMX571 APS-C format native 16-bit ADC sensor. It has an ultra-high 14 stops dynamic range, ultra-low 1.0e readout noise and an innovative breakthrough resulting in zero amp-glow. It is a camera born from the appeal of astrophotography lovers.
Amazing Craftsmanship, Lightweight body, Solid image quality:
We have been working hard to reduce the weight of the camera while improving the performance of the camera. After years of technical accumulation and repeated weight loss experiments by ZWO engineers, ZWO finally concentrated the ASI2600 to 0.7KG.
The ASI2600MM Pro uses APS-C format, the sensor length and width are 23.5mm * 15.7mm and the diagonal is 28.3mm. This is a 26MP camera with a small pixel size of 3.76um that can accommodate a large well depth of 50ke.
Native 16bit ADC:
As one of the few CMOS astronomy cameras with 16bit ADC in the market, ASI2600MM Pro was born with superiorities for astrophotography. This 16bit ADC is not a CCD 16bit ADC. It can really achieve a dynamic range output of 14 stop, which will significantly improve the image sharpness and contrast, also create smoother and more natural color transitions.
IMX571 backlit sensor:
Sony’s back-illuminated CMOS image sensor improves sensitivity and noise reduction – the key factors to enhancing image quality, while radically realigning their fundamental pixel structure from front-illumination to back-illumination. It has retained the advantages of CMOS image sensors such as low power consumption and high-speed operation.
With a conventional front-illumination structure, the metal wiring and transistors on the surface of the silicon substrate that form the sensor’s light-sensitive area (photo-diode) impede photon gathering carried out by the on-chip lens. A back-illuminated structure minimizes the degradation of sensitivity to optical angle response, while also increasing the amount of light that enters each pixel due to the lack of obstacles such as metal wiring and transistors that have been moved to the reverse of the silicon substrate.
Sony has newly developed a unique photo-diode structure and on-chip lens optimized for back-illuminated structures, that achieves a higher sensitivity and a lower random noise without light by reducing noise, dark current and defect pixels compared to the conventional front-illuminated structure.
The ASI2600MM Pro has excellent performance with a dynamic range of up to 14stops. When the gain value is 100, the magical HCG high gain mode is turned on, the readout noise is greatly reduced, and the dynamic range is basically unchanged. For better date quality, it is recommended to set the gain to 0 or gain 100 during deep-sky imaging.
Zero Amp Glow
Traditional CMOS sensors produce a weak infrared light source during operation quite often seen in the corner of uncalibrated images as the tell-tale signs of ‘amp glow’. As the ASI2600MM Pro uses zero amp glow circuitry, you won’t have to worry about amp glow even when using high gain, long exposure imaging.
With amp glow – exposure 300 second exposure
ASI2600 frame with no amp glow – Exposure 300 second
There is a polyimide heater completely fitting the protective window in the ASI2600MM Pro camera. It can help avoid the annoying dew or icing issues.
The power of the heater is around 5W. You are free to turn it off anytime in your photography software if you want to save some power.
According to the test results of Sony, the QE peak value of the ASI2600MM Pro is appr. 91%
Two-stage TEC cooling, ultra-low dark current:
Thanks to the two stage TEC cooling, ASI2600MM Pro can lower the CMOS sensor temperature to more that 35c below ambient, which can greatly reduce dark current generation and sensor noise even with extended exposure times.
The unique dark current suppression technology can even further reduce dark current noise. At a cooling temperature of 0 °, the dark current noise is only 0.0022e/s/pix. Which means 300s exposure can only cause 0.7e dark current noise, which is less than the readout noise. While at a cooling temperature of -20 °, the dark current can even reduce to 0.00012e/s/pix, which is completely negligible!
If you are having any trouble with the cooling, please check out the following page on the manufacturer's website before contacting us:
USB3.0 & 256MB DDR3 Memory Buffer
The ASI2600MM Pro is equipped with a USB 3.0 transmission interface and a built-in 256MB DDR3 cache to ensure stable and secure data transmission. Under long exposure, it effectively avoids frame dropping and greatly reduces the glow effect caused by slow reading speed.
What is in the box?
Notice：Cooled cameras need a 12V power adapter. If you don’t have one, please click this link to buy a 12V power adapter. We will supply it with a cable with UK mains plug.
The best solution of 55mm back focus length
Connection Diagram for dSLR lens:
- Nikon-T2 adapter
- EOS-T2 adapter
- 2” filter (optional)
- Nikon lens
- Canon lens
Drivers and Softwares:
Our website has newest camera drivers and many DSO and Planetary capture softwares. Please make sure the newest driver and software has been installed before you start shooting:
MELOTTE 15 – “THE HEART OF THE HEART NEBULA”
- Subject: Melotte 15 – “The Heart of the Heart Nebula”
- Imaging OTA: Sharpstar SCA260 – 1300mm, f/5.0
- Imaging Camera: ZWO ASI2600MM-PRO
Antlia 2” Narrowband: Ha (3nm); Sii (3.5nm); Oiii (3.5nm)
- Filter Wheel: ZWO 7 x 2”
- Guide System: ZWO OAG-L with ZWO ASI174MM camera
- Capture Details: Ha: 30 x 300s; Sii: 26 x 300s; Oiii: 26 x 300s
- Integration time: 6h40’
- Bortle 4 over 4 nights
Courtesy of Alistair Scobie
(Please note, below is a 900px wide version, but if you click on it, you will see a 1600px wide version. The original was even larger, but we had to reduce it to 1600pixels width as that's the max our shopping cart system allows...)