activity
19942003
collaborators

9 papers

astro-ph2003

Quasar Radio Dichotomy: Two Peaks, or not Two Peaks, that is the Question

Z. Ivezic, G. T. Richards, P. B. Hall +8

Recent claims by Ivezic et al. (2002) that the distribution of the radio-to-optical flux ratio, R, for quasars is bimodal (the so-called quasar radio dichotomy) were questioned on…

astro-ph2003

Counts of Low-redshift SDSS Quasar Candidates

Z. Ivezic, R. H. Lupton, D. E. Johnston +10

We analyze the counts of low-redshift quasar candidates selected using nine-epoch SDSS imaging data. The co-added catalogs are more than 1 mag deeper than single-epoch SDSS data, a…

astro-ph2003

Halo Structure Traced by SDSS RR Lyrae

Z. Ivezic, R. H. Lupton, D. Schlegel +6

We discuss the density and radial velocity distributions of over 3000 candidate RR Lyrae stars selected by various methods using Sloan Digital Sky Survey data for about 1000 deg^2…

astro-ph2001

J-Band Spectroscopy of the z = 5.74 BAL QSO SDSSp J104433.04-012502.2

R. W. Goodrich, R. Campbell, F. Chaffee +8

We use the NIRSPEC near-IR spectrometer on Keck II to obtain moderate resolution (R = 1540) spectroscopy that shows conclusively that the C IV emission line in the z = 5.74 quasar…

astro-ph2001

Extreme BAL Quasars from the Sloan Digital Sky Survey

Patrick B. Hall, J. E. Gunn, G. R. Knapp +16

The Sloan Digital Sky Survey has discovered a population of broad absorption line quasars with various extreme properties. Many show absorption from metastable states of FeII with…

astro-ph2001

The SDSS Imaging Pipelines

Robert Lupton, James E. Gunn, Zeljko Ivezic +3

We summarise the properties of the Sloan Digital Sky Survey (SDSS) project, discuss our software infrastructure, and outline the architecture of the SDSS image processing pipelines…