#Glow free in raya pro 3.0 full

Our camera design has been extensively tested and is very stable.В Even when used in higher humidity environments, ASI294MC Pro will still work well without dew problems. There are four screws that seal the sensor chamber. Reliable MechanicsДЄSI294MC Pro has the same mechanics as ASI1600 Pro. Even bright stars wonвЂ™t saturate under long exposures.В This also means that this camera can achieve higher SNRВ (signal to noise ratio) with just one single exposure.

#Glow free in raya pro 3.0 full

The ASI294MC provides a great full wellВ capacity of 63700e-, which is 3 timesВ higherВ than the capacity of the highly regarded ASI1600. Read noise will drop under 2e-, while dynamic range will remain at 13 stops.

HCG (high conversion gain) mode, which reduces read noise to even lower levels at higher gain without loss to dynamic range, is automatically enabled when the gain setting is 120 or higher.

At 13 stops, the ASI294MCВ has even more dynamic range than the ASI1600. This is an excellent characteristic for deep sky imaging, which inherently needs high dynamic range. The ASI294MC Pro has a 14bit ADC unit, allowing it to achieve 13 stops of dynamic range. Additionally, the use of a memory buffer minimizes amp-glow, which is caused by the slow transfer speeds when the camera is used with a USB 2.0 port.ДDR memory buffer is the main difference between ASI вЂњCoolвЂќ and вЂњProвЂќ cameras. The ASI294MC Pro camera includes a 256MB DDR3 memory buffer to help improve data transfer reliability. This makes the IMX294CJK ideal for astronomic camera market applications that require low-illumination performance. в–¶Exceptional low-illumination performanceД®xceptional low-illumination performance of SNR1s: 0.14 lx is realized by use of a large-size optical system and by expanding the area per pixel to 4.63 Вµm.