The Sloan Digital Sky Survey (SDSS) is an imaging and spectroscopic survey that will
eventually cover approximately one-quarter of the celestial sphere and collect spectra of≈ 10 6 …

The Sloan Digital Sky Survey (SDSS) will provide the data to support detailed investigations
of the distribution of luminous and nonluminous matter in the universe: a photometrically …

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS),
marking the completion of the original goals of the SDSS and the end of the phase known as …

The Low Resolution Imaging Spectrometer (LRIS) for the Cassegrain focus of the Keck 10-m
telescope on Mauna Kea is described. It has an imaging mode so it can also be used for …

The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its Second
Data Release. This data release consists of 3324 deg 2 of five-band (ugriz) imaging data …

The Sloan Digital Sky Survey (SDSS) has validated and made publicly available its First
Data Release. This consists of 2099 deg 2 of five-band (u, g, r, i, z) imaging data, 186,240 …

This paper describes the Fourth Data Release of the Sloan Digital Sky Survey (SDSS),
including all survey-quality data taken through 2004 June. The data release includes five-band …

This paper describes the Third Data Release of the Sloan Digital Sky Survey (SDSS). This
release, containing data taken up through 2003 June, includes imaging data in five bands …

We report the discovery of the coolest field dwarf yet known, selected as an unresolved object
with extremely red colors from commissioning imaging data of the Sloan Digital Sky Survey…

We present photometric and spectroscopic observations of 15 high-redshift quasars (z> 3.6)
discovered from∼ 140 deg 2 of five-color (u &arcmin;, g &arcmin;, r &arcmin;, i &arcmin;, …