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Published online by Cambridge University Press: 25 May 2016
Designing and implementing the Science Archive for the Sloan Digital Sky Survey (Gunn et. al 1992) has presented several unique architectural obstacles. First, the final archive will be large; the cumulative data products will exceed tens of Terabytes. Second, the data will be complex; extracted parameter catalogs will contain links to images, spectra, and objects in other wavelength catalogs. Third, the archive will be widely distributed allowing transparent world-wide access to the available data. Finally, the archive is expected to remain viable well into the next century.