Presentation + Paper
25 July 2024 Simons Observatory: observatory scheduler and automated data processing
Yilun Guan, Kathleen Harrington, Jack Lashner, Sanah Bhimani, Kevin T. Crowley, Nicholas Galitzki, Ken Ganga, Matthew Hasselfield, Adam D. Hincks, Brian Keating, Brian J. Koopman, Laura Newburgh, David V. Nguyen, Max Silva-Feaver
Author Affiliations +
Abstract
The Simons Observatory (SO) is a next-generation ground-based telescope located in the Atacama Desert in Chile, designed to map the cosmic microwave background (CMB) with unprecedented precision. The observatory consists of three Small Aperture Telescopes (SATs) and one Large Aperture Telescope (LAT), each optimized for distinct but complementary scientific goals. To achieve these goals, optimized scan strategies have been defined for both the SATs and LAT. This paper describes a software system deployed in SO that effectively translates high-level scan strategies into realistic observing scripts executable by the telescope, taking into account realistic observational constraints. The data volume of SO also necessitates a scalable software infrastructure to support its daily data processing needs. This paper also outlines an automated workflow system for managing data packaging and daily data reduction at the site.
Conference Presentation
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Yilun Guan, Kathleen Harrington, Jack Lashner, Sanah Bhimani, Kevin T. Crowley, Nicholas Galitzki, Ken Ganga, Matthew Hasselfield, Adam D. Hincks, Brian Keating, Brian J. Koopman, Laura Newburgh, David V. Nguyen, and Max Silva-Feaver "Simons Observatory: observatory scheduler and automated data processing", Proc. SPIE 13101, Software and Cyberinfrastructure for Astronomy VIII, 131010V (25 July 2024); https://doi.org/10.1117/12.3020379
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KEYWORDS
Telescopes

Observatories

Data processing

Automatic control

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