Poster + Paper
31 August 2022 The Simons Observatory: antenna control software integration and implementation
Lauren J. Saunders, Matthew Hasselfield, Brian J. Koopman, Laura Newburgh
Author Affiliations +
Conference Poster
Abstract
The Simons Observatory (SO) is a ground-based cosmic microwave background survey experiment that consists of three 0.5 m small-aperture telescopes and one 6 m large-aperture telescope, sited at an elevation of 5200 m in the Atacama Desert in Chile. SO will study the polarization and temperature anisotropies of the Cosmic Microwave Background (CMB). The observatory will require well-understood telescope pointing and scanning. Good antenna control will allow us to execute the scan strategy devised to optimize sensitivity to our scientific goals, calibrate the system with celestial targets, and make maps. To achieve this, we integrate the data acquisition and control of the telescopes’ Antenna Control Units (ACUs) within the software framework of the SO Observatory Control System (OCS). We present here the current status of the software integration for the ACUs, as well as measurements of the Small Aperture Telescope platforms’ responsiveness to software commanding in the factory, plans for in situ measurements, and prospects for implementation on the Large Aperture Telescope.
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Lauren J. Saunders, Matthew Hasselfield, Brian J. Koopman, and Laura Newburgh "The Simons Observatory: antenna control software integration and implementation", Proc. SPIE 12190, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XI, 121902P (31 August 2022); https://doi.org/10.1117/12.2629724
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KEYWORDS
Telescopes

Data acquisition

Computer programming

Observatories

Control systems

Antennas

Velocity measurements

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