The SOAR Tip-Tilt Guide cameras (TTGC) were built as turnkey systems by Astronomica Research Camera Inc. They are designed around the E2V technologies CCD39-01 CCD which has 80x80 24 microns pixels. This CCD has four very high performance low-readout noise amplifiers and a split-frame transfer architecture, allowing it to be read out at high speed with relatively low noise. The CCD is mounted in a small head including an integral 2-stage Peltier cooler. The CCD is controlled by an SDSU-III controller. It allos the CCD to be read out pixels rates as high as 2 microsec per pixel, allowing the full 80x80 image to be read out at ~240Hz, or a 32x32 pixel guide box to be read out at up to 900Hz while achieveing RON of < 4e- The TTGC is controlled by custom LabVIEW based software developed by Rolando Cantarutti at CTIO. This allows the opperator to set the camera parameters (e.g. frame time, ROI size and binning), provides a real time display of the resulting image, and calculates the position of the guide star and guiding error signal which is used to drive the telescopes fast tertiary steering mirror, and provide slower corrections to the telescope mount in order to stay within the range of correction of the tertiary. The basic performance parameters for the camera are given in the table below:
Actual Guiding performance remains to be characterised at this time. Three seperate TTGC units are currently in use at SOAR, one for each Nasmyth ISB, and one for the SOAR Optical Imager. Because slightly different fore optics are used in each case the scale and field of view differs as shown in the following table.
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