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    Automated data processing architecture for the Gemini Planet Imager Exoplanet Survey

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    018002.pdf
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    Author
    Wang, Jason J. cc
    Perrin, Marshall cc
    Savransky, Dmitry cc
    Arriaga, Pauline cc
    Chilcote, Jeffrey cc
    De Rosa, Robert J. cc
    Millar-Blanchaer, Maxwell A.
    Marois, Christian cc
    Rameau, Julien cc
    Wolff, Schuyler cc
    Shapiro, Jacob
    Ruffio, Jean-Baptiste cc
    Maire, Jérôme
    Marchis, Franck cc
    Graham, James R.
    Macintosh, Bruce cc
    Ammons, S. Mark cc
    Bailey, Vanessa P.
    Barman, Travis S. cc
    Bruzzone, Sebastian
    Bulger, Joanna cc
    Cotten, Tara cc
    Doyon, Rene
    Duchêne, Gaspard cc
    Fitzgerald, Michael P. cc
    Follette, Katherine B.
    Goodsell, Stephen J. cc
    Greenbaum, Alexandra Z.
    Hibon, Pascale
    Hung, Li-Wei
    Ingraham, Patrick cc
    Kalas, Paul
    Konopacky, Quinn cc
    Larkin, James E. cc
    Marley, Mark S. cc
    Metchev, Stanimir
    Nielsen, Eric L.
    Oppenheimer, Rebecca cc
    Palmer, David W.
    Patience, Jennifer
    Poyneer, Lisa A.
    Pueyo, Laurent
    Rajan, Abhijith
    Rantakyro, Fredrik T.
    Schneider, Adam C. cc
    Sivaramakrishnan, Anand cc
    Song, Inseok cc
    Soummer, Remi cc
    Thomas, Sandrine cc
    Wallace, J. Kent
    Ward-Duong, Kimberly
    Wiktorowicz, Sloane J.
    Show allShow less
    Affiliation
    Univ Arizona, Lunar & Planetary Lab, Tucson, AZ 85721 USA
    Issue Date
    2018-01
    Keywords
    high contrast imaging
    exoplanets
    circumstellar disks
    data processing
    Gemini planet imager
    Data Cruncher
    
    Metadata
    Show full item record
    Publisher
    SPIE-SOC PHOTO-OPTICAL INSTRUMENTATION ENGINEERS
    Citation
    Jason J. Wang, Marshall D. Perrin, Dmitry Savransky, Pauline Arriaga, Jeffrey K. Chilcote, Robert J. De Rosa, Maxwell A. Millar-Blanchaer, Christian Marois, Julien Rameau, Schuyler G. Wolff, Jacob Shapiro, Jean-Baptiste Ruffio, Jérôme Maire, Franck Marchis, James R. Graham, Bruce Macintosh, S. Mark Ammons, Vanessa P. Bailey, Travis S. Barman, Sebastian Bruzzone, Joanna Bulger, Tara Cotten, René Doyon, Gaspard Duchêne, Michael P. Fitzgerald, Katherine B. Follette, Stephen Goodsell, Alexandra Z. Greenbaum, Pascale Hibon, Li-Wei Hung, Patrick Ingraham, Paul Kalas, Quinn M. Konopacky, James E. Larkin, Mark S. Marley, Stanimir Metchev, Eric L. Nielsen, Rebecca Oppenheimer, David W. Palmer, Jennifer Patience, Lisa A. Poyneer, Laurent Pueyo, Abhijith Rajan, Fredrik T. Rantakyrö, Adam C. Schneider, Anand Sivaramakrishnan, Inseok Song, Remi Soummer, Sandrine Thomas, J. Kent Wallace, Kimberly Ward-Duong, Sloane J. Wiktorowicz, “Automated data processing architecture for the Gemini Planet Imager Exoplanet Survey,” J. Astron. Telesc. Instrum. Syst. 4(1), 018002 (2018), doi: 10.1117/1.JATIS.4.1.018002.
    Journal
    JOURNAL OF ASTRONOMICAL TELESCOPES INSTRUMENTS AND SYSTEMS
    Rights
    © 2018 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
    The Gemini Planet Imager Exoplanet Survey (GPIES) is a multiyear direct imaging survey of 600 stars to discover and characterize young Jovian exoplanets and their environments. We have developed an automated data architecture to process and index all data related to the survey uniformly. An automated and flexible data processing framework, which we term the Data Cruncher, combines multiple data reduction pipelines (DRPs) together to process all spectroscopic, polarimetric, and calibration data taken with GPIES. With no human intervention, fully reduced and calibrated data products are available less than an hour after the data are taken to expedite follow up on potential objects of interest. The Data Cruncher can run on a supercomputer to reprocess all GPIES data in a single day as improvements are made to our DRPs. A backend MySQL database indexes all files, which are synced to the cloud, and a front-end web server allows for easy browsing of all files associated with GPIES. To help observers, quicklook displays show reduced data as they are processed in real time, and chatbots on Slack post observing information as well as reduced data products. Together, the GPIES automated data processing architecture reduces our workload, provides real-time data reduction, optimizes our observing strategy, and maintains a homogeneously reduced dataset to study planet occurrence and instrument performance. (c) 2018 Society of Photo-Optical Instrumentation Engineers (SPIE)
    ISSN
    2329-4124
    DOI
    10.1117/1.JATIS.4.1.018002
    Version
    Final published version
    Sponsors
    NASA's NExSS program [NNX15AD95G]; Office of Science of the U.S. Department of Energy [DE-AC02-05CH11231]; National Science Foundation [ACI-1548562]; NASA through Hubble Fellowship - Space Telescope Science Institute [51378.01-A]; NASA [NAS5-26555]; U.S. Department of Energy by Lawrence Livermore National Laboratory [DE-AC52-07NA27344]
    Additional Links
    https://www.spiedigitallibrary.org/journals/Journal-of-Astronomical-Telescopes-Instruments-and-Systems/volume-4/issue-01/018002/Automated-data-processing-architecture-for-the-Gemini-Planet-Imager-Exoplanet/10.1117/1.JATIS.4.1.018002.full
    ae974a485f413a2113503eed53cd6c53
    10.1117/1.JATIS.4.1.018002
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