A Map of the Northern Sky: The Sloan Digital Sky Survey in Its First Year

Eva K. Grebel

Published 2001-05-09Version 1

The Sloan Digital Sky Survey (SDSS) is the largest and most ambitious optical CCD survey undertaken to date. It will ultimately map out one quarter of the sky with precision photometry in five bands, high-quality astrometry, and spectra of all galaxies and quasars brighter than certain limiting magnitudes. The scientific potential of the SDSS is enormous and addresses a wide variety of astrophysical key questions. After a proprietary period the reduced and calibrated data are made available to the astronomical community as a whole. The SDSS is run by an international consortium involving universities and research institutions. One of the participating partners is the Max Planck Institute for Astronomy in Heidelberg. Already in its first year the SDSS has led to a number of spectacular scientific discoveries. In this paper, we will introduce the SDSS survey, discuss its scientific potential, highlight important science results, and present the Calar Alto key program for SDSS follow-up studies.