paper

The Sloan Digital Sky Survey

arXiv:astro-ph/9805314 · doi:10.1098/rsta.1999.0316

Abstract

The Sloan Digital Sky Survey is an ambitious, multi-institutional project to create a huge digital imaging and spectroscopic data bank of 25% of the celestial sphere, approximately 10,000 deg^2 centred on the north galactic polar cap. The photometric atlas will be in 5 specially-chosen colours, covering the pi ster of the Survey area to a limiting magnitude of r~23.1, on 0.4" pixels, resulting in a 1 Tpixel map. This data base will be automatically analysed to catalog the photometric and astrometric properties of 10^8 stellar images, 10^8 galaxies, and 10^6 colour-selected QSO candidates; the galaxy data will in addition include detailed morphological data. The photometric data are used to autonomously and homogeneously select objects for the spectroscopic survey, which will include spectra of 10^6 galaxies, 10^5 QSOs, and 10^5 unusual stars. Although the project was originally motivated by the desire to study Large Scale Structure, we anticipate that these data will impact virtually every field of astronomy, from Earth-crossing asteroids to QSOs at z>6. In particular, the ~12 TByte multi-colour, precision calibrated imaging archive should be a world resource for many decades of the next century.

On behalf of the entire scientific and technical team of the Survey. Paper presented at "Discussion Meeting on Large Scale Structure in the Universe," Royal Society, London, March 1998; 11 pages including 2 figures and no tables. To appear in Philosophical Transactions of the Royal Society of London A, 1998. Requires LaTeX and rspublic.sty. Revised version: typos corrected, very slight additions, references updated

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