Poster + Paper
16 August 2024 The Simons Observatory: deployment and current configuration of the observatory control system for SAT-MF1 and data access software systems
Sanah Bhimani, Jack Lashner, Simone Aiola, Kevin T. Crowley, Nicholas Galitzki, Kathleen Harrington, Matthew Hasselfield, Alyssa Johnson, Brian J. Koopman, Hironobu Nakata, Laura Newburgh, David V. Nguyen, Michael J. Randall, Max Silva-Feaver
Author Affiliations +
Conference Poster
Abstract
The Simons Observatory (SO) is a Cosmic Microwave Background experiment located in the Atacama Desert in Chile. SO consists of three small aperture telescopes (SATs) and one large aperture telescope (LAT) with a total of 60,000 detectors in six frequency bands.1 As an observatory, SO encompasses hundreds of hardware components simultaneously running at different readout rates—all separate from its 60,000 detectors on-sky and their metadata. We provide an overview of commissioning SO’s data acquisition software system for SAT-MF1, the first SAT deployed to the Atacama site. Additionally, we share insights from deploying data access software for all four telescopes, detailing how performance limitations affected data loading and quality investigations, which led to site-compatible software improvements.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Sanah Bhimani, Jack Lashner, Simone Aiola, Kevin T. Crowley, Nicholas Galitzki, Kathleen Harrington, Matthew Hasselfield, Alyssa Johnson, Brian J. Koopman, Hironobu Nakata, Laura Newburgh, David V. Nguyen, Michael J. Randall, and Max Silva-Feaver "The Simons Observatory: deployment and current configuration of the observatory control system for SAT-MF1 and data access software systems", Proc. SPIE 13102, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy XII, 131021B (16 August 2024); https://doi.org/10.1117/12.3020237
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KEYWORDS
Telescopes

Data acquisition

Observatories

Databases

Environmental monitoring

Cryogenics

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