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XPipeline: Starlight subtraction at scale for MagAO-X

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arxiv 2208.07354 v1 pith:4GNJAPCH submitted 2022-08-15 astro-ph.IM

XPipeline: Starlight subtraction at scale for MagAO-X

classification astro-ph.IM
keywords datadevelopedexaohighmagao-xpost-processingscalescience
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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MagAO-X is an extreme adaptive optics (ExAO) instrument for the Magellan Clay 6.5-meter telescope at Las Campanas Observatory in Chile. Its high spatial and temporal resolution can produce data rates of 1 TB/hr or more, including all AO system telemetry and science images. We describe the tools and architecture we use for commanding, telemetry, and science data transmission and storage. The high data volumes require a distributed approach to data processing, and we have developed a pipeline that can scale from a single laptop to dozens of HPC nodes. The same codebase can then be used for both quick-look functionality at the telescope and for post-processing. We present the software and infrastructure we have developed for ExAO data post-processing, and illustrate their use with recently acquired direct-imaging data.

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