Section 4 - Camera Hardware
4.Camera Hardware
This section describes the modular components that make up the CCD Camera System and how they fit into the observatory, with all their connections to power and other equipment.
4.1.System Components
The
The CCDs, Preamplifier, and Readout Electronics are mounted in the front of the optical head. The optical head interfaces to the telescope through a 1.25 inch draw tube, sliding into the telescope's focus mechanism. The placement of the preamplifier and readout electronics close to the CCD is necessary to achieve good noise performance. The Microcontroller is housed in the rear of the Optical Head along with the interface logic to the PC and Telescope.
4.2.Connecting the Power
The desktop power supply is designed to run off wall voltage, and both domestic (110 VAC) and European (220 VAC) versions are available. In the field however, battery operation may be the most logical choice. In that case you need to use the optional 12V power supply or a 12VDC to 110 VAC power inverter.
4.3.Connecting to the Computer
The
4.4.Connecting the Relay Port to the Telescope
The
In the Track mode and Self Guided mode the host software corrects the telescope as often as once every 2 seconds to compensate for drift in the mount and drive system. The host software and the CCD camera operate in tandem to repeatedly take exposures of the designated guide star, calculate its position to a tenth of a pixel accuracy, and then automatically activate the telescope's controller to move the star right back to its intended position. It does this tirelessly to guide long duration astrophotographs.
In the Track and Accumulate mode the software takes a series of images and automatically
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