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4-m Prime Focus CCD (1Mar93) (from CTIO, NOAO Newsletter No. 33, 1 March 1993) The new Large-Format PFCCD imager was completed on schedule and went for its first engineering run on December 18. It is designed to accommodate CCDs or mosaics up to 75 mm square, and has two filter wheels capable of holding five 102 mm square filters. The CCDTV camera is on a stage which permits short-scanning, while there are facilities for easy tilt and rotation of the dewar so that large CCDs can be accurately aligned with the focal plane. It works either with the triplet correctors or with the soon-to-be-installed ADC. Instrument control uses DC or DC servo motors via a STD-Bus box. Apart from the ability to use large CCDs at the 4-m, the images are expected to be significantly improved (especially with the ADC) since the present arrangement has the CCD centered well off-axis of the doublet corrector. The above-mentioned engineering night was also the first on which an ARCON-based controller had been tried at the 4-m telescope, and it was also the first time a CCDTV camera had been used at PF for acquisition and guiding. Installation went extremely smoothly, focussing took place soon after dark, and by 2 AM all the engineers had vanished! The equipment functioned well, but some system integration work remains to be done to make all the computers (ARCON, TCS, Motor-control) talk (and listen) to each other. With the red triplet and a CCD with 0.35 arcsec pixels, the images had 1.1-1.3 arcsec FWHM on a night when the other telescopes reported 1.5-1.7 arcsec FWHM, whereas on following nights with the old PFCCD system the FWHM was the same as the other telescopes. This rather meager statistic suggests that image quality has improved with the new system. Another engineering night is scheduled in February, and it is hoped that the instrument will be available for visitor use starting with the April prime focus run. Alistair Walker, Tom Ingerson, Andres Montane, Javier Rojas, Rodolfo Cardemil
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