The SDSS Imaging Pipelines

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dc.creatorLupton, Robert
dc.creatorGunn, James E.
dc.creatorIvezic, Zeljko
dc.creatorKnapp, Gillian R.
dc.creatorKent, Stephen
dc.creatorYasuda, Naoki
dc.date2001-01-23
dc.date2001-05-24
dc.date.accessioned2026-07-07T01:57:29Z
dc.date.available2026-07-07T01:57:29Z
dc.descriptionWe summarise the properties of the Sloan Digital Sky Survey (SDSS) project, discuss our software infrastructure, and outline the architecture of the SDSS image processing pipelines. We then discuss two of the algorithms used in the SDSS image processing; the KL-transform based modelling of the spatial variation of the PSF, and the use of galaxy models in star/galaxy separation. We conclude with the first author's personal opinions on the challenges that the astronomical community faces with major software projects.
dc.description10 pages, 4 figures. Submitted to ADASS X conference; uses adassconf.sty Added author; minor editorial changes
dc.identifierhttps://arxiv.org/abs/astro-ph/0101420
dc.identifierhttp://arxiv.org/abs/astro-ph/0101420
dc.identifierASP Conf.Ser. 10 (2001) 269
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2404
dc.subjectAstrophysics
dc.titleThe SDSS Imaging Pipelines
dc.typetext

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