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20042026
most citedModeling the Time Variability of SDSS Stripe 82 Quasars as a Damped Random Walk

705 citations · 4.4k across the 51 of their papers we have counts for

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6 papers · 1 filter

astro-ph2008★ 170 cited

A Unified Catalog of Radio Objects Detected by NVSS, FIRST, WENSS, GB6, and SDSS

Amy E. Kimball, Željko Ivezić

(Abridged) We construct a catalog of radio sources detected by the GB6 (6 cm), FIRST and NVSS (20 cm), and WENSS (92 cm) radio surveys, and the SDSS optical survey. The 2.7 million…

astro-ph2008★ 573 cited

The Milky Way Tomography with SDSS: II. Stellar Metallicity

Zeljko Ivezic, Branimir Sesar, Mario Juric +50

Using effective temperature and metallicity derived from SDSS spectra for ~60,000 F and G type main sequence stars (0.2<g-r<0.6), we develop polynomial models for estimating these…

astro-ph2007★ 436 cited

Stellar SEDs from 0.3-2.5 Microns: Tracing the Stellar Locus and Searching for Color Outliers in SDSS and 2MASS

Kevin R. Covey, Zeljko Ivezic, David J. Schlegel +15

The Sloan Digital Sky Survey (SDSS) and Two Micron All Sky Survey (2MASS) are rich resources for studying stellar astrophysics and the structure and formation history of the Galaxy…

astro-ph2007★ 1 cited

SDSS spectroscopic survey of stars

Z. Ivezic, D. Schlegel, A. Uomoto +37

In addition to optical photometry of unprecedented quality, the Sloan Digital Sky Survey (SDSS) is also producing a massive spectroscopic database. We discuss determination of stel…

astro-ph2005★ 33 cited

The UV, Optical, and IR Properties of SDSS Sources Detected by GALEX

Marcel A. Agueros, Zeljko Ivezic, Kevin R. Covey +18

We discuss the UV, optical, and IR properties of the SDSS sources detected by GALEX as part of its All-sky Imaging Survey Early Release Observations. Virtually all of the GALEX sou…

astro-ph2004★ 185 cited

Measurement of Galaxy Cluster Sizes, Radial Profiles, and Luminosity Functions from SDSS Photometric Data

Sarah M. Hansen, Timothy A. McKay, Risa H. Wechsler +3

Imaging data from the Sloan Digital Sky Survey is used to measure the empirical size-richness relation for a large sample of galaxy clusters. Using population subtraction methods,…