By popular demand, we now introduce the ASI294MM Pro. This is the monochrome version of the ASI294MC Pro – one of the top selling cameras from ZWO. Some of the highlights include: Back-illuminated sensor – improving sensitivity and reducing noise; 4/3” format with 4.64 um pixel size – ideal for many types of telescopes

As ZWO’s latest BSI (backside illuminated type) mono camera, ASI294MM has very high QE performance, not only higher than its color version, but even ASI1600MM. It is estimated that the QE peak value is about 90% .

ZWO ASI294MC-Pro cooled color astronomy camera uses micro-4/3 Sony IMX294CJK CMOS sensor; High 4144x2822 resolution (11.7 megapixels) and 4.63-micron pixel size; Ideal for capturing high-resolution color astronomical images of extended brighter deep-sky objects and lunar/solar/planetary images

2017年10月17日 · The dark current of 294 is a little bit higher than 1600 from out test result. ASI294 VS ASI1600. Let’s see this table to compare the difference between 294 and 1600 camera: In sum, ASI294MC Pro have much potential, 14bit ADC, 63700e full well, 1.2e read noise, DDR buffer, each feature means a new posibility! This camera is available now!

作为zwo最受欢迎的彩色冷冻相机的黑白版本，asi294mm pro的各项参数和asi294mc pro都很接近，维持了一贯的优越水准，但不仅如此，黑白版本还在满阱大小和qe数值上超越了一大步。

Welcome to join ZWO FB and User Forum below! Facebook : https://www.facebook.com/ZwoDesignAstronomyCameras User Forum: https://bbs.astronomy-imaging-camera.com/ ASI294 Camera is specifically designed for astronomical photography. It is not only suitable for DSO imaging but also for Planetary imaging. You will be impressed by its …

2021年2月15日 · The ZWO ASI1294MC features Sony's remarkable IMG294CJK 4/3 CMOS sensor with a massive 4144x2822 resolution! That's over 11 megapixels!

2021年1月26日 · The ZWO ASI 294MM Pro has a large well depth capacity, low read-out noise and high dynamic range. The full well capacity of 66387e of ASI 294MM Pro is among the best ASI DSO cameras. It ensures a very high dynamic range of up to 13 stops, which significantly reduces overexposure probability and helps achieve richer colour gradation.