activity
20032009
most citedLSST Science Book, Version 2.0

924 citations · 1.8k across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2009★ 924 cited

LSST Science Book, Version 2.0

LSST Science Collaboration, Paul A. Abell, Julius Allison +245

A survey that can cover the sky in optical bands over wide fields to faint magnitudes with a fast cadence will enable many of the exciting science opportunities of the next decade.…

astro-ph2008★ 6 cited

Time Variability of Quasars: the Structure Function Variance

C. MacLeod, Z. Ivezic, W. de Vries +2

Significant progress in the description of quasar variability has been recently made by employing SDSS and POSS data. Common to most studies is a fundamental assumption that photom…

astro-ph2008★ 311 cited

From Shock Breakout to Peak and Beyond: Extensive Panchromatic Observations of the Type Ib Supernova 2008D associated with Swift X-ray Transient 080109

Maryam Modjaz, W. Li, N. Butler +38

We present extensive early photometric (ultraviolet through near-infrared) and spectroscopic (optical and near-infrared) data on supernova (SN) 2008D as well as X-ray data analysis…

astro-ph2007★ 28 cited

Star-Formation in Low Radio Luminosity AGN from the Sloan Digital Sky Survey

W. H. de Vries, J. A. Hodge, R. H. Becker +2

We investigate faint radio emission from low- to high-luminosity Active Galactic Nuclei (AGN) selected from the Sloan Digital Sky Survey (SDSS). Their radio properties are inferred…

astro-ph2007★ 32 cited

Imaging and Spectroscopy of Ultra Steep Spectrum Radio Sources

Carlos G. Bornancini, Carlos De Breuck, Wim de Vries +4

We present a sample of 40 Ultra Steep Spectrum (USS, , ) radio sources selected from the Westerbork in the Southern Hemisphere (WISH) catalog. The USS s…

astro-ph2006★ 24 cited

XMM-NEWTON Detection of X-ray Emission from the Compact Steep Spectrum Radio Galaxy 3C303.1

C. O'Dea, B. Mu, D. Worrall +3

Using XMM we detect faint unresolved X-ray emission from the Compact Steep Spectrum radio galaxy 3C303.1. We detect a thermal component at kT = 0.8 keV which seems likely to be pro…