Active Optics - 'Large Format'*please note imaging camera or guide camera in photos and diagrams not included
The SXV-AO-LF active optics system provides excellent Image stability to give best results with most optical systems and mounts by using a high speed tip-tilt optical window to overcome rapid gear errors. It is very effective at stabilising the effects of even difficult mounts. The AO assembly uses an off-axis autoguider, such as the SXV guide head, and provides accurate positional feedback to the control software. High Speed corrections of the star field postion are generated and applied, without any need to move the mount, thus avoiding the delays associated with conventional guiding.
Unlike cameras with an integrated guider chip, the OAG puts the guide camera ahead of any filters that the user fits into the recess provided and so guiding sensitivity is always at maximum.
The guide camera mounting is designed to be parfocal with an SX camera when used in this combination - fine focus adjustment is provided by moving the threaded guider mount along the prism tube. If you do not need the OAG barrel (e.g when using a camera with a built-in OAG or guide chip), you can fit the 72mm or T adaptor directly onto the rear of the AO assembly. The normal AO OAG unit is not required for this option.
Major Features of the AO-LF
The SXV-AOLF should be used with the off-axis guider assembly for the best results with most optical systems. This combination uses an SXV guide head or Lodestar to view the edge of the telescope field via a 10mm square prism and provides accurate positional feedback to the control software.
A side view of the AOLF assembly.
The SXV-AOLF can also be used with the 'Ultraslim' OAG and filter wheel assembly. In this case, you do not need the OAG for the AO unit, just the T mount adaptor to connect the AO to the OAG, as seen above. You will save about 27mm of back focal length if you use this method.
STAR2000 cameras may be used directly without the OAG, but the AO correction rate must be kept reasonably slow, or amplifier glow effects may become a serious issue.
A front view, showing the imaging and guide camera CCDs, along with the input and output connections.
Some examples of the AO in use
No processing was applied, other than cropping, so that the images are essentially 'raw'. The mount used was a Celestron CI700 with a C11 SCT at F10
A 2x enlarged clip from an SXV-H9 image. Ten minutes with a C11 at F10 using mount guiding only.
Another clip taken a few minutes later with the AO switched on and operating at 3 updates per second.
Here are some 'extreme' images from an Ultima 2000 on a fork mount with poor polar alignment and rapid gear errors. The camera was an SXV-M8C and the images have been resampled to 50% of full size for display.
Without AO correction.
With the AO switched on. (The short coloured spikes on the bright stars were produced when the AO switched off for image download)