Spectral Reduction Software for the DEEP2 Redshift Survey

Details Spectral Reduction Software for the DEEP2 Redshift Survey Spectral Reduction Software for the DEEP2 Redshift Survey

2001-09-10

arxiv.org/abs/astro-ph/0109164v1

Astronomy and Astrophysics

Astrophysics

To appear in the proceedings of the Marseille 2001 conference "Where is the Matter? Tracing Dark and Bright Matter with the Ne

Scientific paper

The 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.

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