Paper 13094-145
No photon left behind: optimizing image quality for the Argus Optical Array
Abstract
Argus Pathfinder is a wide-field optical survey designed to discover transient events via sub-minute deep imaging. Pathfinder integrates up to 38 small-aperture telescopes into a single tracking mount and is also a 1:20 scale prototype for the planned 900-telescope all-sky Argus Optical Array. Optimizing and maintaining image quality for this many optical assemblies is challenging. Each assembly must be carefully collimated, tilt-aligned, and focused to micron-level precision and remain stable over months-long timescales. These calibrations will be achieved with a custom focuser design coupled with robotic actuation and dedicated software tools and preserved by operating the array in a lab-like enclosure, limiting the need for cleaning and maintenance. We present the performance of Argus Pathfinder’s climate-control system (in continuous operation for a year as of December 2023), our custom focuser design, and the development of the automated calibration process tested on Pathfinder for full deployment on the Argus Optical Array.
Presenter
Lawrence M. Machia
The Univ. of North Carolina at Chapel Hill (United States)
Lawrence Machia is a 4th year astrophysics PhD candidate at the University of North Carolina, Chapel Hill where he works under Dr. Nicholas Law as a member of the Argus Pathfinder and Argus Optical Array team. His current scientific interests include astronomical instrumentation, exoplanet habitability, and multi-messenger astronomy. Lawrence is also a Roman Catholic priest (6 years) and a Benedictine monk (11 years) of Saint Vincent Archabbey in Latrobe, PA. He has a deep interest in the history and philosophy of science, and after graduating expects to continue his research and career at Saint Vincent College located at his monastery.