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Design and Implementation of Data Reduction Pipelines for the Keck Observatory Archive

Gelino, Christopher R. and Berriman, G. B. and Kong, M. and Laity, A. C. and Swain, M. A. and Campbell, R. and Goodrich, R. W. and Holt, J. and Lyke, J. and Mader, J. A. and Tran, H. D. and Barlow, T. (2015) Design and Implementation of Data Reduction Pipelines for the Keck Observatory Archive. In: Astronomical Data Analysis Software and Systems XXIV. Astronomical Society of the Pacific conference series. No.495. Astronomical Society of the Pacific , San Francisco, CA, pp. 359-362. ISBN 9781583818749. https://resolver.caltech.edu/CaltechAUTHORS:20160324-105613919

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Abstract

The Keck Observatory Archive (KOA), a collaboration between the NASA Exoplanet Science Institute and the W. M. Keck Observatory, serves science and calibration data for all active and inactive instruments from the twin Keck Telescopes located near the summit of Mauna Kea, Hawaii. In addition to the raw data, we produce and provide quick look reduced data for four instruments (HIRES, LWS, NIRC2, and OSIRIS) so that KOA users can more easily assess the scientific content and the quality of the data, which can often be difficult with raw data. The reduced products derive from both publicly available data reduction packages (when available) and KOA-created reduction scripts. The automation of publicly available data reduction packages has the benefit of providing a good quality product without the additional time and expense of creating a new reduction package, and is easily applied to bulk processing needs. The downside is that the pipeline is not always able to create an ideal product, particularly for spectra, because the processing options for one type of target (eg., point sources) may not be appropriate for other types of targets (eg., extended galaxies and nebulae). In this poster we present the design and implementation for the current pipelines used at KOA and discuss our strategies for handling data for which the nature of the targets and the observers' scientific goals and data taking procedures are unknown. We also discuss our plans for implementing automated pipelines for the remaining six instruments.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
http://www.aspbooks.org/a/volumes/article_details/?paper_id=37357PublisherArticle
ORCID:
AuthorORCID
Berriman, G. B.0000-0001-8388-534X
Campbell, R.0000-0002-3289-5203
Additional Information:© 2015 Astronomical Society of the Pacific. KOA is collaboration between the W. M. Keck Observatory (WMKO) and the NASA Exoplanet Science Institute (NExScI). Funding for KOA is provided by NASA. WMKO is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA.
Group:Infrared Processing and Analysis Center (IPAC)
Funders:
Funding AgencyGrant Number
NASAUNSPECIFIED
Series Name:Astronomical Society of the Pacific conference series
Issue or Number:495
Record Number:CaltechAUTHORS:20160324-105613919
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20160324-105613919
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:65655
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:30 Mar 2016 23:41
Last Modified:09 Mar 2020 13:18

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