ZWO ASI2600MC Pro Cooled Color Astronomy Camera
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Please note: This ZWO Pro/Cooled camera must be powered from an external 12V DC power source with a minimum of 3 amps in order to run the TEC cooler and connect to your computer. The camera may not be recognized by a computer or operate properly if only the USB3.0 cable is connected to your computer. You can use ZWO’s 12V DC power supply, the DC Out port on a ZWO ASIAir or an external battery. These are not included with the camera.
The ZWO ASI2600MC Pro: The Perfect Solution for One-Shot Color Astrophotography
ZWO has been a leader in the astrophotography market since the release of its legendary ASI1600MM monochrome and ASI1600MC color astronomy cameras. And this newest generation of cooled astronomy cameras continues to lead the pack. The ZWO ASI2600MC has set a new standard for deep space astrophotography using one-shot color cameras, with its cutting-edge technology, and it’s large, back-illuminated Sony IMX571 APS-C sensor.
These new CMOS sensors deliver an impressive resolution of 26-megapixels with a native 16-bit ADC, allowing it to capture rich details across a wide dynamic range. The ZWO ASI2600MC Pro uses an innovative two-stage TEC cooling system, further improving the low-noise design of its CMOS sensor. All of this means that your images will end up having so little dark-current noise that many astrophotographers skip taking dark frames for post-processing!
Additional features include an anti-dew heater, a high-speed USB 3.0 interface, and an onboard DDR3 cache. These ensure robust performance and efficient data handling, making the ZWO ASI2600MC a standout choice for astrophotographers seeking reliable, high-quality color cameras for deep sky astrophotography.
ZWO ASI2600MC Pro Review
Check out Agena Astro affiliate Peter Zelinka's detailed review of the ZWO ASI2600MC Pro, after using it for 6 months. He shares his hands-on experience, highlighting the camera's performance, features, and how it stands up to real-world astrophotography.
ZWO ASI2600MC Key Performance Features
- 26 Megapixel Full-Frame Sensor: Delivers exceptional high-resolution detail for capturing deep-sky objects with precision.
- True 16-bit ADC: Provides up to 14 stops of high dynamic range, ensuring excellent contrast and detail in both bright and dark areas.
- 80% Peak Quantum Efficiency (QE): Greater sensitivity means more light capture, resulting in clearer and more detailed images.
- 50ke- Full Well Capacity: Prevents saturation of bright stars, even in long exposures.
- Ultra-Low Readout Noise (1.0e - 3.3e): Enhances image clarity and dynamic range.
- Zero Amp-Glow: Ensures clean, noise-free images, even during extended exposures, reducing post-processing hassle.
- Seamless Compatibility with ZWO Accessories: Integrates effortlessly with accessories like the ZWO CAA Camera Angle Adjuster Electronic Rotator, the ZWO 7-Position Electronic Filter Wheel for 2" Filters (EFW), and the ZWO OAG-L Large Off-Axis Guider with 1.25" Holder (OAG-L).
ASI2600MC Pro: Exceptional Image Quality with Advanced Sensor Technology
High-Resolution Astrophotography
The ZWO ASI2600MC Pro is a dedicated, cooled, one-shot color astronomy camera with an extremely sensitive CMOS sensor — the famed Sony IMX571. With a sensor array of 6248 x 4176 pixels in an APS-C format, this high-resolution deep sky imaging camera offers 26-megapixels for extremely detailed astrophotography. This means you can print your images, enlarge them, or crop them to your heart's content!
Clearer Images with Zero Amp Glow
A significant change in this generation of CMOS sensors is the complete removal of any traces of amp glow. Amp-glow is when a typically weak infrared light source leaks onto your sensor and leaves a pattern or shape on the final images. This issue affects many older astronomy cameras, DSLRs, and even newer mirrorless cameras. Most cases are severe enough that your dark frames need their own set of flats to properly calibrate. Thankfully the ASI2600MC Pro does not experience this issue at all, making calibration and post-processing a breeze!
Dual Gain Structure For Greater Sensitivity
Apart from the disappearance of amp glow, another notable evolution from previous generations of astronomy cameras is the dual gain structure used by the Sony IMX571. This means that at a gain of 100, the read noise plummets, and the dynamic range improves to allow for pristine images. Even at higher gains, the ASI2600MC maintains improved sensitivity, better detail, and reduced noise. While ZWO recommends a gain of 100 for most uses, you can adjust this setting as needed based on the target or set-up you’re using.
Essential features of the ZWO ASI2600MC Pro
Top-Tier Technical Specifications
The ASI2600MC Pro features some of the best technical capabilities of any astrophotography camera currently available to consumers. It has a QE of over 80%. This means more than 80% of the light that hits your sensor is recorded as data. This is essential when imaging faint objects in deep space. The ASI2600MC Pro also has an ADC of 16 bits allowing for a very wide dynamic range, as well as an impressively large full well capacity of 50,000e. This means that each pixel can record a high amount of information without clipping your precious data, as has been the case with some previous generations of CMOS sensors.
Backside-Illuminated Sensor (BSI)
Sony has been developing their backside-illumination sensor (BSI) technology for a while now. This technology greatly improves overall sensitivity and noise reduction. Traditional camera sensors include all of the essential electronics on top of the silicon layer of the sensor. This design blocks some of the light from reaching the sensor, so BSI sensors flip this design and move all the electronics to the back of the silicon layer. This gives the photons a clear path straight to the light-sensitive area of the camera sensor, which improves the sensor's ability to capture light coming in from different angles. It also provides better overall sensitivity across the full visible spectrum of light.
This is particularly important for high-resolution sensors like the IMX571. It is also crucial for ZWO’s larger full-frame models, the ASI6200MM, ASI6200MC, and ASI2400MC.
The importance grows even more when accounting for the larger file sizes of a 16-bit sensor. When combined with the low-noise CMOS architecture of these modern sensors, BSI technology helps to create images with such low-noise they barely need calibration frames!
Native 16-bit ADC
The ASI2600MC continues to set itself apart with a sophisticated 16-bit analog-to-digital converter (ADC). Unlike traditional CCD cameras that might claim 16-bit capability but fall short, this new-generation CMOS sensor delivers a true 14-stop dynamic range. For astrophotographers, this means the ability to capture the faintest wisps of nebulosity and the brightest star cores in a single frame. This isn’t just another stat to pad the numbers - it translates into noticeably sharper images with richer contrast and beautifully smooth tonal transitions, especially when using narrowband filters. This makes the ASI2600 Pro one of the few cameras in its class that can truly handle the extreme brightness range of deep-sky imaging.
Two-stage TEC Cooling
The ASI2600MM Pro's powerful two-stage cooling system can drop the sensor by a massive -31ºF (-35ºC) below the ambient temperature. This dramatically reduces unwanted thermal noise during long deep-sky exposures. While this cooling system is highly effective, it’s only one part of ZWO’s approach to reducing noise.
The ZWO ASI2600MC also uses innovative dark current suppression technology. When cooled to 0°C, the camera produces a mere 0.0022 electrons of dark current noise per second per pixel. To put this into perspective, even during a 5-minute exposure, the total dark current noise (0.7e) remains lower than the camera's base readout noise! Cool the sensor down to -20°C, and the dark current becomes virtually non-existent at 0.00012e/s/pixel - making it so low it's essentially irrelevant to your final image quality.
Please note: the camera’s TEC cooler requires a 12V external power supply (not included).
USB 3.0 for High-Speed Data Transfer
The ASI2600MC Pro is equipped with a high-speed USB 3.0 interface and a built-in 256MB DDR3 cache, both of which ensure stable and secure data transmission. During long exposures, this combination effectively avoids frame dropping and significantly reduces the “glow” effect caused by slow readout speed.
Additional Info
The best solutions to reach a 55mm back focus length:
What are the power and setup requirements?
The ASI2600MC-P requires an external 11–14V power source to operate, even if the cooler isn’t active. This can be an external power supply or the power outputs from an ASIAir. This design ensures the cooling system and all internal electronics work reliably.
What sensor and performance characteristics does it offer?
The ZWO ASI260MC Pro is equipped with Sony’s back‐illuminated IMX571 APS-C format sensor. This sensor provides a native 16-bit ADC, high dynamic range (up to 14 stops), 26MP resolution with a pixel size of 3.76µm, and a full well depth of 50ke. These features help capture fine details while keeping noise to a minimum.
How does the two-stage TEC cooling and noise performance work?
The ASI2600MC-P incorporates a two-stage TEC cooling system that can lower the sensor temperature to more than 35°C below ambient. This cooling dramatically reduces dark current noise, and the innovative “zero amp glow” design further minimizes unwanted artifacts during long exposures.
What distinguishes the color (ASI2600MC-P) version from the monochrome model?
Both models share essentially the same sensor technology and performance benefits, with the main difference being a QE of 80% on the color version versus 91% on the monochrome version. Color astronomy cameras are typically chosen for ease of use and because of their lower cost and easier post-processing routines.
How do I achieve proper integration with my telescope setup?
ZWO includes all the necessary spacers and adapters to connect with any system that requires 55mm of backspacing and which uses M42 or m48 threads. Please see the included diagrams for reaching optimal spacing using the included parts.
What measures are in place for robust data transmission?
To address concerns about data reliability, the ZWO ASI2600MC Pro uses a USB 3.0 interface along with an in-camera DDR3 cache (512MB in models produced after August 2023). This system ensures that large volumes of data are handled smoothly, even during extended imaging sessions.
How is dew or icing managed during cold nights of imaging?
The ZWO ASI2600MC-Pro is equipped with a polyimide heater that fits over the protective window of the sensor. This actively helps to reduce dew or icing in the camera, thereby ensuring consistent performance and clear images through long exposures.
Other Information
- Country of Manufacture: China
The ZWO ASI2600MC Pro: The Perfect Solution for One-Shot Color Astrophotography
ZWO has been a leader in the astrophotography market since the release of its legendary ASI1600MM monochrome and ASI1600MC color astronomy cameras. And this newest generation of cooled astronomy cameras continues to lead the pack. The ZWO ASI2600MC has set a new standard for deep space astrophotography using one-shot color cameras, with its cutting-edge technology, and it’s large, back-illuminated Sony IMX571 APS-C sensor.
These new CMOS sensors deliver an impressive resolution of 26-megapixels with a native 16-bit ADC, allowing it to capture rich details across a wide dynamic range. The ZWO ASI2600MC Pro uses an innovative two-stage TEC cooling system, further improving the low-noise design of its CMOS sensor. All of this means that your images will end up having so little dark-current noise that many astrophotographers skip taking dark frames for post-processing!
Additional features include an anti-dew heater, a high-speed USB 3.0 interface, and an onboard DDR3 cache. These ensure robust performance and efficient data handling, making the ZWO ASI2600MC a standout choice for astrophotographers seeking reliable, high-quality color cameras for deep sky astrophotography.
ZWO ASI2600MC Pro Review
Check out Agena Astro affiliate Peter Zelinka's detailed review of the ZWO ASI2600MC Pro, after using it for 6 months. He shares his hands-on experience, highlighting the camera's performance, features, and how it stands up to real-world astrophotography.
ZWO ASI2600MC Key Performance Features
- 26 Megapixel Full-Frame Sensor: Delivers exceptional high-resolution detail for capturing deep-sky objects with precision.
- True 16-bit ADC: Provides up to 14 stops of high dynamic range, ensuring excellent contrast and detail in both bright and dark areas.
- 80% Peak Quantum Efficiency (QE): Greater sensitivity means more light capture, resulting in clearer and more detailed images.
- 50ke- Full Well Capacity: Prevents saturation of bright stars, even in long exposures.
- Ultra-Low Readout Noise (1.0e - 3.3e): Enhances image clarity and dynamic range.
- Zero Amp-Glow: Ensures clean, noise-free images, even during extended exposures, reducing post-processing hassle.
- Seamless Compatibility with ZWO Accessories: Integrates effortlessly with accessories like the ZWO CAA Camera Angle Adjuster Electronic Rotator, the ZWO 7-Position Electronic Filter Wheel for 2" Filters (EFW), and the ZWO OAG-L Large Off-Axis Guider with 1.25" Holder (OAG-L).
ASI2600MC Pro: Exceptional Image Quality with Advanced Sensor Technology
High-Resolution Astrophotography
The ZWO ASI2600MC Pro is a dedicated, cooled, one-shot color astronomy camera with an extremely sensitive CMOS sensor — the famed Sony IMX571. With a sensor array of 6248 x 4176 pixels in an APS-C format, this high-resolution deep sky imaging camera offers 26-megapixels for extremely detailed astrophotography. This means you can print your images, enlarge them, or crop them to your heart's content!
Clearer Images with Zero Amp Glow
A significant change in this generation of CMOS sensors is the complete removal of any traces of amp glow. Amp-glow is when a typically weak infrared light source leaks onto your sensor and leaves a pattern or shape on the final images. This issue affects many older astronomy cameras, DSLRs, and even newer mirrorless cameras. Most cases are severe enough that your dark frames need their own set of flats to properly calibrate. Thankfully the ASI2600MC Pro does not experience this issue at all, making calibration and post-processing a breeze!
Dual Gain Structure For Greater Sensitivity
Apart from the disappearance of amp glow, another notable evolution from previous generations of astronomy cameras is the dual gain structure used by the Sony IMX571. This means that at a gain of 100, the read noise plummets, and the dynamic range improves to allow for pristine images. Even at higher gains, the ASI2600MC maintains improved sensitivity, better detail, and reduced noise. While ZWO recommends a gain of 100 for most uses, you can adjust this setting as needed based on the target or set-up you’re using.
Essential features of the ZWO ASI2600MC Pro
Top-Tier Technical Specifications
The ASI2600MC Pro features some of the best technical capabilities of any astrophotography camera currently available to consumers. It has a QE of over 80%. This means more than 80% of the light that hits your sensor is recorded as data. This is essential when imaging faint objects in deep space. The ASI2600MC Pro also has an ADC of 16 bits allowing for a very wide dynamic range, as well as an impressively large full well capacity of 50,000e. This means that each pixel can record a high amount of information without clipping your precious data, as has been the case with some previous generations of CMOS sensors.
Backside-Illuminated Sensor (BSI)
Sony has been developing their backside-illumination sensor (BSI) technology for a while now. This technology greatly improves overall sensitivity and noise reduction. Traditional camera sensors include all of the essential electronics on top of the silicon layer of the sensor. This design blocks some of the light from reaching the sensor, so BSI sensors flip this design and move all the electronics to the back of the silicon layer. This gives the photons a clear path straight to the light-sensitive area of the camera sensor, which improves the sensor's ability to capture light coming in from different angles. It also provides better overall sensitivity across the full visible spectrum of light.
This is particularly important for high-resolution sensors like the IMX571. It is also crucial for ZWO’s larger full-frame models, the ASI6200MM, ASI6200MC, and ASI2400MC.
The importance grows even more when accounting for the larger file sizes of a 16-bit sensor. When combined with the low-noise CMOS architecture of these modern sensors, BSI technology helps to create images with such low-noise they barely need calibration frames!
Native 16-bit ADC
The ASI2600MC continues to set itself apart with a sophisticated 16-bit analog-to-digital converter (ADC). Unlike traditional CCD cameras that might claim 16-bit capability but fall short, this new-generation CMOS sensor delivers a true 14-stop dynamic range. For astrophotographers, this means the ability to capture the faintest wisps of nebulosity and the brightest star cores in a single frame. This isn’t just another stat to pad the numbers - it translates into noticeably sharper images with richer contrast and beautifully smooth tonal transitions, especially when using narrowband filters. This makes the ASI2600 Pro one of the few cameras in its class that can truly handle the extreme brightness range of deep-sky imaging.
Two-stage TEC Cooling
The ASI2600MM Pro's powerful two-stage cooling system can drop the sensor by a massive -31ºF (-35ºC) below the ambient temperature. This dramatically reduces unwanted thermal noise during long deep-sky exposures. While this cooling system is highly effective, it’s only one part of ZWO’s approach to reducing noise.
The ZWO ASI2600MC also uses innovative dark current suppression technology. When cooled to 0°C, the camera produces a mere 0.0022 electrons of dark current noise per second per pixel. To put this into perspective, even during a 5-minute exposure, the total dark current noise (0.7e) remains lower than the camera's base readout noise! Cool the sensor down to -20°C, and the dark current becomes virtually non-existent at 0.00012e/s/pixel - making it so low it's essentially irrelevant to your final image quality.
Please note: the camera’s TEC cooler requires a 12V external power supply (not included).
USB 3.0 for High-Speed Data Transfer
The ASI2600MC Pro is equipped with a high-speed USB 3.0 interface and a built-in 256MB DDR3 cache, both of which ensure stable and secure data transmission. During long exposures, this combination effectively avoids frame dropping and significantly reduces the “glow” effect caused by slow readout speed.
- ZWO ASI2600MC Pro Camera Body
- Soft Case
- Quick Guide
- USB 3.0 Cable (2 meter)
- 2x USB 2.0 Cable (0.5 meter)
- T2 - M48 Extender (16.5mm)
- T2 Extender (21mm)
- M42 to M48 Adapter
- Dust Cover
- Hexagon Wrench
Please note: This ZWO Pro/Cooled camera must be powered from an external 12V DC power source with a minimum of 3 amps in order to run the TEC cooler and connect to your computer. The camera may not be recognized by a computer or operate properly if only the USB3.0 cable is connected to your computer. You can use ZWO’s 12V DC power supply, the DC Out port on a ZWO ASIAir or an external battery. These are not included with the camera.
The ZWO ASI2600MC Pro: The Perfect Solution for One-Shot Color Astrophotography
ZWO has been a leader in the astrophotography market since the release of its legendary ASI1600MM monochrome and ASI1600MC color astronomy cameras. And this newest generation of cooled astronomy cameras continues to lead the pack. The ZWO ASI2600MC has set a new standard for deep space astrophotography using one-shot color cameras, with its cutting-edge technology, and it’s large, back-illuminated Sony IMX571 APS-C sensor.
These new CMOS sensors deliver an impressive resolution of 26-megapixels with a native 16-bit ADC, allowing it to capture rich details across a wide dynamic range. The ZWO ASI2600MC Pro uses an innovative two-stage TEC cooling system, further improving the low-noise design of its CMOS sensor. All of this means that your images will end up having so little dark-current noise that many astrophotographers skip taking dark frames for post-processing!
Additional features include an anti-dew heater, a high-speed USB 3.0 interface, and an onboard DDR3 cache. These ensure robust performance and efficient data handling, making the ZWO ASI2600MC a standout choice for astrophotographers seeking reliable, high-quality color cameras for deep sky astrophotography.
ZWO ASI2600MC Pro Review
Check out Agena Astro affiliate Peter Zelinka's detailed review of the ZWO ASI2600MC Pro, after using it for 6 months. He shares his hands-on experience, highlighting the camera's performance, features, and how it stands up to real-world astrophotography.
ZWO ASI2600MC Key Performance Features
- 26 Megapixel Full-Frame Sensor: Delivers exceptional high-resolution detail for capturing deep-sky objects with precision.
- True 16-bit ADC: Provides up to 14 stops of high dynamic range, ensuring excellent contrast and detail in both bright and dark areas.
- 80% Peak Quantum Efficiency (QE): Greater sensitivity means more light capture, resulting in clearer and more detailed images.
- 50ke- Full Well Capacity: Prevents saturation of bright stars, even in long exposures.
- Ultra-Low Readout Noise (1.0e - 3.3e): Enhances image clarity and dynamic range.
- Zero Amp-Glow: Ensures clean, noise-free images, even during extended exposures, reducing post-processing hassle.
- Seamless Compatibility with ZWO Accessories: Integrates effortlessly with accessories like the ZWO CAA Camera Angle Adjuster Electronic Rotator, the ZWO 7-Position Electronic Filter Wheel for 2" Filters (EFW), and the ZWO OAG-L Large Off-Axis Guider with 1.25" Holder (OAG-L).
ASI2600MC Pro: Exceptional Image Quality with Advanced Sensor Technology
High-Resolution Astrophotography
The ZWO ASI2600MC Pro is a dedicated, cooled, one-shot color astronomy camera with an extremely sensitive CMOS sensor — the famed Sony IMX571. With a sensor array of 6248 x 4176 pixels in an APS-C format, this high-resolution deep sky imaging camera offers 26-megapixels for extremely detailed astrophotography. This means you can print your images, enlarge them, or crop them to your heart's content!
Clearer Images with Zero Amp Glow
A significant change in this generation of CMOS sensors is the complete removal of any traces of amp glow. Amp-glow is when a typically weak infrared light source leaks onto your sensor and leaves a pattern or shape on the final images. This issue affects many older astronomy cameras, DSLRs, and even newer mirrorless cameras. Most cases are severe enough that your dark frames need their own set of flats to properly calibrate. Thankfully the ASI2600MC Pro does not experience this issue at all, making calibration and post-processing a breeze!
Dual Gain Structure For Greater Sensitivity
Apart from the disappearance of amp glow, another notable evolution from previous generations of astronomy cameras is the dual gain structure used by the Sony IMX571. This means that at a gain of 100, the read noise plummets, and the dynamic range improves to allow for pristine images. Even at higher gains, the ASI2600MC maintains improved sensitivity, better detail, and reduced noise. While ZWO recommends a gain of 100 for most uses, you can adjust this setting as needed based on the target or set-up you’re using.
Essential features of the ZWO ASI2600MC Pro
Top-Tier Technical Specifications
The ASI2600MC Pro features some of the best technical capabilities of any astrophotography camera currently available to consumers. It has a QE of over 80%. This means more than 80% of the light that hits your sensor is recorded as data. This is essential when imaging faint objects in deep space. The ASI2600MC Pro also has an ADC of 16 bits allowing for a very wide dynamic range, as well as an impressively large full well capacity of 50,000e. This means that each pixel can record a high amount of information without clipping your precious data, as has been the case with some previous generations of CMOS sensors.
Backside-Illuminated Sensor (BSI)
Sony has been developing their backside-illumination sensor (BSI) technology for a while now. This technology greatly improves overall sensitivity and noise reduction. Traditional camera sensors include all of the essential electronics on top of the silicon layer of the sensor. This design blocks some of the light from reaching the sensor, so BSI sensors flip this design and move all the electronics to the back of the silicon layer. This gives the photons a clear path straight to the light-sensitive area of the camera sensor, which improves the sensor's ability to capture light coming in from different angles. It also provides better overall sensitivity across the full visible spectrum of light.
This is particularly important for high-resolution sensors like the IMX571. It is also crucial for ZWO’s larger full-frame models, the ASI6200MM, ASI6200MC, and ASI2400MC.
The importance grows even more when accounting for the larger file sizes of a 16-bit sensor. When combined with the low-noise CMOS architecture of these modern sensors, BSI technology helps to create images with such low-noise they barely need calibration frames!
Native 16-bit ADC
The ASI2600MC continues to set itself apart with a sophisticated 16-bit analog-to-digital converter (ADC). Unlike traditional CCD cameras that might claim 16-bit capability but fall short, this new-generation CMOS sensor delivers a true 14-stop dynamic range. For astrophotographers, this means the ability to capture the faintest wisps of nebulosity and the brightest star cores in a single frame. This isn’t just another stat to pad the numbers - it translates into noticeably sharper images with richer contrast and beautifully smooth tonal transitions, especially when using narrowband filters. This makes the ASI2600 Pro one of the few cameras in its class that can truly handle the extreme brightness range of deep-sky imaging.
Two-stage TEC Cooling
The ASI2600MM Pro's powerful two-stage cooling system can drop the sensor by a massive -31ºF (-35ºC) below the ambient temperature. This dramatically reduces unwanted thermal noise during long deep-sky exposures. While this cooling system is highly effective, it’s only one part of ZWO’s approach to reducing noise.
The ZWO ASI2600MC also uses innovative dark current suppression technology. When cooled to 0°C, the camera produces a mere 0.0022 electrons of dark current noise per second per pixel. To put this into perspective, even during a 5-minute exposure, the total dark current noise (0.7e) remains lower than the camera's base readout noise! Cool the sensor down to -20°C, and the dark current becomes virtually non-existent at 0.00012e/s/pixel - making it so low it's essentially irrelevant to your final image quality.
Please note: the camera’s TEC cooler requires a 12V external power supply (not included).
USB 3.0 for High-Speed Data Transfer
The ASI2600MC Pro is equipped with a high-speed USB 3.0 interface and a built-in 256MB DDR3 cache, both of which ensure stable and secure data transmission. During long exposures, this combination effectively avoids frame dropping and significantly reduces the “glow” effect caused by slow readout speed.
Additional Info
The best solutions to reach a 55mm back focus length:
What are the power and setup requirements?
The ASI2600MC-P requires an external 11–14V power source to operate, even if the cooler isn’t active. This can be an external power supply or the power outputs from an ASIAir. This design ensures the cooling system and all internal electronics work reliably.
What sensor and performance characteristics does it offer?
The ZWO ASI260MC Pro is equipped with Sony’s back‐illuminated IMX571 APS-C format sensor. This sensor provides a native 16-bit ADC, high dynamic range (up to 14 stops), 26MP resolution with a pixel size of 3.76µm, and a full well depth of 50ke. These features help capture fine details while keeping noise to a minimum.
How does the two-stage TEC cooling and noise performance work?
The ASI2600MC-P incorporates a two-stage TEC cooling system that can lower the sensor temperature to more than 35°C below ambient. This cooling dramatically reduces dark current noise, and the innovative “zero amp glow” design further minimizes unwanted artifacts during long exposures.
What distinguishes the color (ASI2600MC-P) version from the monochrome model?
Both models share essentially the same sensor technology and performance benefits, with the main difference being a QE of 80% on the color version versus 91% on the monochrome version. Color astronomy cameras are typically chosen for ease of use and because of their lower cost and easier post-processing routines.
How do I achieve proper integration with my telescope setup?
ZWO includes all the necessary spacers and adapters to connect with any system that requires 55mm of backspacing and which uses M42 or m48 threads. Please see the included diagrams for reaching optimal spacing using the included parts.
What measures are in place for robust data transmission?
To address concerns about data reliability, the ZWO ASI2600MC Pro uses a USB 3.0 interface along with an in-camera DDR3 cache (512MB in models produced after August 2023). This system ensures that large volumes of data are handled smoothly, even during extended imaging sessions.
How is dew or icing managed during cold nights of imaging?
The ZWO ASI2600MC-Pro is equipped with a polyimide heater that fits over the protective window of the sensor. This actively helps to reduce dew or icing in the camera, thereby ensuring consistent performance and clear images through long exposures.
Other Information
- Country of Manufacture: China
- ZWO ASI2600MC Pro Camera Body
- Soft Case
- Quick Guide
- USB 3.0 Cable (2 meter)
- 2x USB 2.0 Cable (0.5 meter)
- T2 - M48 Extender (16.5mm)
- T2 Extender (21mm)
- M42 to M48 Adapter
- Dust Cover
- Hexagon Wrench