Section 4 - Camera Hardware
required is that with most modern telescope mounts the drift over the relatively short 1 minute interval is small enough to preserve round star images, a feat that even the best telescope mounts will not maintain over the longer ten minute interval. The Track and Accumulate software does allow correction of the telescope position in the interval between snapshots to keep the guide star grossly positioned within the field of view, but it is the precise co- registration of images that accounts for the streakless images.
The host software and the CCD camera control the telescope through the
Note: You only need to interface the camera's Telescope port to your telescope if you are planning on using the camera system as an autoguider or selfguider, or feel you need to have the Track and Accumulate command make telescope corrections between images because your drive has a large amount of long term drift.
Some recent model telescopes (like the Celestron Ultima and the Meade LX200) have connectors on the drive controller that interface directly to the camera's TTL level Telescope port. All that's required is a simple cable to attach the 9 pin Telescope port to the telescope's telephone jack type CCD connector. SBIG includes its
4.4.1 Using Mechanical Relays
Older telescopes generally require modifying the hand controller to accept input from the camera's Telescope port. The difficulty of this task varies with the drive corrector model and may require adding external relays if your drive corrector will not accept TTL level signals. We maintain a database of instructions for the more popular telescopes that we will gladly share with you. For a minimal charge will also modify your hand controllers if you feel you do not have the skills necessary to accomplish such a task. We sell a mechanical relay box that interfaces to the
In general, the camera has four signals that are used in tracking applications. There is one output line for each of the four correction directions on the hand controller (North, South, East and West). Our previous cameras had internal relays for the telescope interface, but with the proliferation of TTL input telescopes the relays were removed in the
In our older camera models and in the optional relay adapter accessory, each of the relays has a Common, a Normally Open, and a Normally Closed contact. For example, when
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