Jon Loveday, Jeff Pier
Published 1998-09-14Version 1
The Sloan Digital Sky Survey (SDSS) will carry out a digital photometric and spectroscopic survey over pi steradians in the northern Galactic cap. An array of CCD detectors used in drift-scan mode will image the sky in five passbands to a limiting magnitude of r' ~ 23. Selected from the imaging survey, 10^6 galaxies, 10^5 quasars and selected samples of stars will be observed spectroscopically. In addition, a smaller (225 deg^2), deeper, southern survey will reach ~2.0 magnitudes fainter and will contain a wealth of information about variable sources, supernovae and proper motions. We describe the current status of the survey, which recently saw first light, and its prospects for constraining cosmological models.
Comments: 6 pages, 1 embedded figure. To appear in proceedings of the 14th IAP meeting "Wide field surveys in cosmology", ed. Y. Mellier et al
The Sloan Digital Sky Survey: Status and Prospects
The Sloan Digital Sky Survey and dark matter
Two-Dimensional Topology of the Sloan Digital Sky Survey
