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We describe the development of new low-noise feeds to upgrade the receiver systems on the Allen Telescope Array (ATA) (Welch et al. 2009). The array consists of 42 antennas distributed over a few acres of land at the Hat Creek Radio Observatory in Northern California. Each antenna utilizes a 6.1 meter diameter primary reflector and a 2.4 meter secondary with offset Gregorian optics to minimize the interference scattered into the system.
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