Spectral Reduction Software for the DEEP2 Redshift Survey

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dc.creatorMarinoni, Christian
dc.creatorDavis, Marc
dc.creatorCoil, Alison L.
dc.creatorFinkbeiner, Douglas
dc.date2001-09-10
dc.date.accessioned2026-07-07T01:59:55Z
dc.date.available2026-07-07T01:59:55Z
dc.descriptionThe DEEP2/DEIMOS redshift survey, which will begin observing in the Spring of 2002, will gather high quality spectra on ~60000 galaxies in order to study the evolution of the properties and large scale clustering of galaxies at z~1. The data rate from DEIMOS will be in excess of 1 Gbyte/hour, and it is therefore imperative to employ completely automated data reduction techniques to manage the analysis. We here describe aspects of our data pipeline, which will make extensive use of B-splines for the sky-subtraction stage and for the combination of multiple frames.
dc.descriptionTo appear in the proceedings of the Marseille 2001 conference "Where is the Matter? Tracing Dark and Bright Matter with the New Generation of Large-Scale Surveys"s
dc.identifierhttps://arxiv.org/abs/astro-ph/0109164
dc.identifierhttp://arxiv.org/abs/astro-ph/0109164
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3306
dc.subjectAstrophysics
dc.titleSpectral Reduction Software for the DEEP2 Redshift Survey
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