What is HCG mode on the Player One Artemis-C Pro?
High Conversion Gain (HCG) mode is an internal camera setting that automatically activates at a gain of 120. There the camera has 12.97 stops of dynamic range, a 14.5k e- full well and 1.8e readout noise, against 13 stops, 65.8k e- and 7.8e at gain 0.
How does the 65.8k full well of the Artemis-C Pro benefit imaging the Orion Nebula (M42)?
The core of M42 around the Trapezium is far brighter than the outer nebula. At gain 0 the Artemis-C Pro has a 65.8k e- full well and 13 stops of dynamic range, so bright areas take longer to saturate in each sub-exposure; many imagers still add short exposures for the core.
What is the difference between the 17.5mm and 12.5mm back focus options on the Artemis-C Pro?
Back focus is the distance from the camera's front flange to the sensor. The Artemis-C Pro offers two options:
-
17.5mm: This is the standard distance with the sensor tilt plate installed. Player One's BFL solution drawings show how to reach the usual spacing.
-
12.5mm: This shorter distance is achieved by removing the sensor tilt plate.
Does the Player One Artemis-C Pro require an external power supply?
Yes, for cooling. With only the main Type-C port connected, the camera works as an uncooled camera. However, to activate the 2-stage TEC cooling system, you must connect a 12V DC power supply (not included) with a minimum rating of 5A to the 5.5x2.1mm power port. The cooler's maximum power draw is 3A.
What does the 4-point tilt adjuster on the Artemis-C Pro do?
It lets you square the sensor to your telescope's light path. A tilt plate gives a much smaller field curvature when imaging deep-sky objects, and with 4 points it is easier to know which corner needs adjusting. It is adjusted from the rear.
Is the 512MB DDR3 buffer on the Artemis-C Pro important?
Yes. The 512 MB DDR3 cache stabilizes data transmission, effectively avoids frame dropping and greatly reduces readout noise, and with it the camera still performs very well on a USB 2.0 port.