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The Atacama Large Millimeter/submillimeter Array (ALMA) is a joint project between astronomical organizations in
Europe, North America, and East Asia, in collaboration with the Republic of Chile. ALMA will consist of at least 54
twelve-meter antennas and 12 seven-meter antennas operating as an interferometer in the millimeter and sub-millimeter
wavelength range. It will be located at an altitude above 5000m in the Chilean Atacama desert. As part of the ALMA
construction phase the Assembly, Verification and Integration (AIV) team receives antennas and instrumentation from
Integrated Product Teams (IPTs), verifies that the sub-systems perform as expected, performs the assembly and
integration of the scientific instrumentation and verifies that functional and performance requirements are met. This
paper aims to describe those aspects related to the AIV Engineering team, its role within the 4-station AIV process, the
different phases the group underwent, lessons learned and potential space for improvement.
AIV Engineering initially focused on the preparation of the necessary site infrastructure for AIV activities, on the
purchase of tools and equipment and on the first ALMA system installations. With the first antennas arriving on site the
team started to gather experience with AIV Station 1 beacon holography measurements for the assessment of the overall
antenna surface quality, and with optical pointing to confirm the antenna pointing and tracking capabilities. With the
arrival of the first receiver AIV Station 2 was developed which focuses on the installation of electrical and cryogenic
systems and incrementally establishes the full connectivity of the antenna as an observing platform. Further antenna
deliveries then allowed to refine the related procedures, develop staff expertise and to transition towards a more routine
production process. Stations 3 and 4 deal with verification of the antenna with integrated electronics by the AIV Science
Team and is not covered directly in this paper. It is believed that both continuous improvement and the clear definition of
the AIV 4-station model were key factors in achieving the goal of bringing the antennas into a state that is well enough
characterized in order to smoothly start commissioning activities.
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