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WIYN Moves Toward Operation in 1994 (1Sep93) (from KPNO, NOAO Newsletter No. 35, 1 September 1993) The WIYN Project is on schedule for early scientific operations and shared-risk observing in late 1994; much progress has been made since the report in the June Newsletter. The alt-azimuth telescope mount was shipped to Kitt Peak in mid-May. Teams from the WIYN Project, NOAO/KPNO, and the manufacturer, L&F Industries, were involved in the on-site assembly. Installation of the major structure took place in the week of 17-22 May. The telescope drives, limit switches, brakes, and encoders were also installed during that period. Dummy weights for the primary and secondary mirror assemblies were used to balance the Optics Support Structure in elevation, and the azimuth, elevation, and instrument rotator axes were tested. The current effort at the Observatory centers around cabling and preparing for installation of the controls. The University of Wisconsin delivered the telescope servo amplifiers and power supplies in June and tested them under manual control. At that time ethernet cabling was installed throughout the building. Installation of the telescope control computers is scheduled for August, after which time closed loop testing of the drives will begin. The NOAO Primary Mirror Group continues fabrication and assembly of the mirror cell and supports. The mirror supports are being assembled as parts arrive from suppliers. Work on the electronics and controls for the active supports is well underway and on schedule. Plans for integrating the mirror assembly with the WIYN telescope are being coordinated with the WIYN Project staff. Work on the thermal control has centered primarily on the assembly of the chiller that supplies conditioned water to the heat exchangers in the cell. Contraves is polishing the 1.2-m secondary mirror for WIYN. By mid-June a 5 wave peak-valley surface finish was achieved using profilometry to guide the figuring. A metrology mount and test optics have been fabricated, and interferometric testing is expected to start in July. In the meantime, fabrication of the secondary mirror cell is well underway at NOAO and is expected to be complete prior to delivery of the mirror. Work on the 1.1-m tertiary mirror at Kodak is nearing completion pending results of the final tests. The mirror was initially polished to 1 wave peak-to-valley on Kodak's large planetary polisher and then placed in their ion polisher for two finish runs. Delivery is expected in July or August. The tertiary mirror cell design is complete and ready for fabrication following completion of the secondary mirror cell. Both the secondary and tertiary mirrors will be supported using a common pressure/vacuum system. For the secondary, the space behind the mirror will be partially evacuated to support its weight. An air bag will be provided for the tertiary. The pressure/vacuum system has been prototyped and is under test at NOAO. The tertiary mirror assembly is supported by the primary mirror cell through the central hole in the primary mirror. A rotator and tilt mechanism allows the telescope beam to be directed to any one of three instrument ports. This mechanism and associated structure is being fabricated by L&F Industries with delivery expected in August. The design of the 1 degree wide-field corrector for use with the Multi-Object Spectrometer (MOS) has been finalized, and fabrication is scheduled to start in August. The MOS will be semi-permanently mounted on one of the two Nasmyth instrument rotators. The other Nasmyth focus will be available for various other instruments including a CCD imager. Science instruments at that focus will mount on an adapter box (IAS) that will provide target acquisition, guiding, atmospheric dispersion compensation, wavefront sensing for active optics, and spectral calibration sources. A critical design review on the IAS was held 28 June. Under the current schedule, telescope commissioning will start early in CY 1994. Planning for the commissioning and operations phases is underway. Matt Johns, Caty Pilachowski
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