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    XPipeline: Starlight subtraction at scale for MagAO-X

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    Author
    Long, J.D.
    Males, J.R.
    Haffert, S.Y.
    Close, L.M.
    Morzinski, K.M.
    van Gorkom, K.
    Lumbres, J.
    Foster, W.
    Hedglen, A.
    Kautz, M.
    Rodack, A.
    Schatz, L.
    Miller, K.
    Doelman, D.
    Bos, S.
    Kenworthy, M.A.
    Snik, F.
    Otten, G.P.P.L.
    Show allShow less
    Affiliation
    Steward Observatory, University of Arizona
    Wyant College of Optical Sciences, University of Arizona
    Issue Date
    2022-08-29
    Keywords
    coronagraphy
    high-performance computing
    post-processing
    
    Metadata
    Show full item record
    Publisher
    SPIE
    Citation
    Joseph D. Long, Jared R. Males, Sebastiaan Y. Haffert, Laird M. Close, Katie M. Morzinski, Kyle Van Gorkom, Jennifer Lumbres, Warren Foster, Alexander Hedglen, Maggie Kautz, Alex Rodack, Lauren Schatz, Kelsey Miller, David Doelman, Steven P. Bos, Matthew A. Kenworthy, Frans Snik, Gilles P. P. L. Otten, "XPipeline: starlight subtraction at scale for MagAO-X," Proc. SPIE 12185, Adaptive Optics Systems VIII, 121853P (29 August 2022); https://doi.org/10.1117/12.2628975
    Journal
    Proceedings of SPIE - The International Society for Optical Engineering
    Rights
    © 2022 SPIE. (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE).
    Collection Information
    This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.
    Abstract
    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. © 2022 SPIE.
    Note
    Immediate access
    ISSN
    0277-786X
    ISBN
    978-151065351-1
    DOI
    10.1117/12.2628975
    Version
    Final Published Version
    ae974a485f413a2113503eed53cd6c53
    10.1117/12.2628975
    Scopus Count
    Collections
    UA Faculty Publications

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