Presentation
28 August 2024 The Argus Array: low-cost access to the deep, high-cadence sky
Nicholas Law, Hank Corbett, Alan Vasquez Soto, Ramses Gonzalez, Lawrence Machia, Jonathan Carney, William Marshall, Glenn Walters, Shannon Fitton, Amy Glazier, Thomas Procter
Author Affiliations +
Abstract
The Argus Array will be the first large optical telescope capable of exploring the entire sky simultaneously. Consisting of 900 small-aperture telescopes with ultra-low-noise detectors multiplexed into a 55 GPix array, Argus will have the equivalent collecting area of a 5m telescope but will explore the sky in a very different way from conventional survey telescopes. Each Argus exposure covers 8,000 square degrees with a sampling of 1.4"/pixel; this enormous field of view allows the Array to achieve deep imaging by observing every part of the sky at cadences as fast as one second – for 6-10 hours each night. Realtime transient detection systems will process the incoming images at TB/sec speeds on a high-speed GPU cluster. Over five years, the Array will build a publicly-available, two-color, million-epoch movie of the northern sky, giving the astronomical community the unprecedented ability to follow the evolution of every deep time-variable source across the sky simultaneously. We will detail the current status of the Argus project, including construction plans and first results from the on-sky Argus Pathfinder hardware and software prototype system.
Conference Presentation
© (2024) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Nicholas Law, Hank Corbett, Alan Vasquez Soto, Ramses Gonzalez, Lawrence Machia, Jonathan Carney, William Marshall, Glenn Walters, Shannon Fitton, Amy Glazier, and Thomas Procter "The Argus Array: low-cost access to the deep, high-cadence sky", Proc. SPIE 13094, Ground-based and Airborne Telescopes X, 130941W (28 August 2024); https://doi.org/10.1117/12.3019797
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