4 Considerations for Imaging
The Gemini system has many features that make it especially suitable as an imaging
platform. These include polar alignment tools, multiple tracking rates, guiding modes, an
autoguider input, and a very sophisticated set of Periodic Error Control (PEC) functions.
This chapter describes how to take full advantage of your Gemini when imaging.
4.1 Accuracy of Polar Alignment
As mentioned previously, accurate polar alignment is extremely important when imaging.
Even through Gemini' s pointing model and closed loop tracking can compensate for
inaccurate polar alignment, photographs and CCD images can be ruined by field rotation.
Gemini' s Polar Axis Correction function helps you achieve sufficiently accurate polar
alignment for all but the longest wide field images, for which only the technique of drift
alignment is likely to suffice.
4.2 Guiding
Theoretically, good polar alignment and the appropriate tracking rate (such as the
adaptive King rate) should be enough to keep the telescope pointing at an object
throughout a long exposure. In reality, however, mechanical imperfections, alignment
errors and other factors will cause the telescope to stray slightly from perfect tracking.
This can result in stars being trailed or bloated, or otherwise distorted in an image. To
overcome this problem, most astrophotographers guide their mounts for exposures over a
minute or two. This involves making occasional slight adjustments to the RA and Dec.
so that a star (or the object being photographed) stays in exactly the same spot in the
telescope' s field of view throughout the exposure. Guiding corrections can be made
manually using buttons on a Hand Controller, or automatically using a CCD autoguider.
In both cases, these corrections are fed into the Gemini system, which actually moves the
mount.
You can set the speed at which guiding corrections are made using the Setup
Mount
Parameters
Moving Speeds
Guiding menu item. You can select a guiding rate
between 0.2x sidereal and 0.8x sidereal. While the guiding occurs at a constant speed
north or south in Dec., it is added to or subtracted from the tracking speed (1x sidereal) in
RA. The RA drive always tracks the telescope to the west; it just speeds up or slows
down when it receives a guiding correction. The standard Guiding Speed is 0.5x, giving
0.5x and 1.5x sidereal speed in RA. The highest guiding speed is 0.8x, giving
approximately 0.8x tracking speed in Dec., and 0.2x and 1.8x in RA.
4.2.1 The Autoguider Port
IMPORTANT:
There are two different versions of the Gemini Autoguider port
hardware. The versions can be distinguished by the type of connectors used for the motor
cables. The older Gemini version uses RJ 45 modular connectors, and the newer version
uses 6 pin DIN connectors. The primary difference between the versions is that the older
Gemini Users Manual
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