ALMA North American Integration Center Front-End Test System
Geoffrey A. Ediss, Joshua Crabtree, Kirk Crady, Erik Gaines, Morgan, McLeod, Greg Morris, Rick Williams, Antonio Perfetto, and John Webber

TL;DR
This paper details the design and performance testing of the ALMA North American Front-End Test System, ensuring quality control for the complex array of receivers used in the ALMA observatory.
Contribution
It introduces a specialized test system for verifying ALMA Front End units, enhancing quality assurance before deployment.
Findings
Test system effectively verifies Front End performance.
Improved sensitivity and reliability of ALMA receivers.
Supports timely delivery of high-quality units.
Abstract
The Atacama Large Millimeter/submillimeter (ALMA) Array Front End (FE) system is the first element in a complex chain of signal receiving, conversion, processing and recording. 70 Front Ends will be required for the project. The Front End is designed to receive signals in ten different frequency bands. In the initial phase of operations, the antennas will be fully equipped with six bands. These are Band 3 (84-116 GHz), Band 4 (125-163 GHz), Band 6 (211-275 GHz), Band 7 (275-373 GHz), Band 8 (385-500 GHz) and Band 9 (602-720 GHz). It is planned to equip the antennas with the missing bands at a later stage of ALMA operations, with a few Band 5 (163-211 GHz) and Band 10 (787-950 GHz) receivers in use before the end of the construction project. The ALMA Front End is far superior to any existing receiver systems; spin-offs of the ALMA prototypes are leading to improved sensitivities in…
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