activity
19992008
most citedThe Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

314 citations · 593 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph2008★ 21 cited

Probing Spectroscopic Variability of Galaxies & Narrow-Line Active Galactic Nuclei in the Sloan Digital Sky Survey

Ching-Wa Yip, Andrew Connolly, Daniel Vanden Berk +10

Under the unified model for active galactic nuclei (AGNs), narrow-line (Type 2) AGNs are, in fact, broad-line (Type 1) AGNs but each with a heavily obscured accretion disk. We woul…

astro-ph2004★ 314 cited

The Galaxy-mass Correlation Function Measured from Weak Lensing in the SDSS

E. S. Sheldon, D. E. Johnston, J. A. Frieman +8

We present galaxy-galaxy lensing measurements over scales 0.025 to 10 Mpc/h in the Sloan Digital Sky Survey. Using a flux-limited sample of 127,001 lens galaxies with spectroscopic…

astro-ph2003★ 53 cited

Physical Evidence for Dark Energy

R. Scranton, A. J. Connolly, R. C. Nichol +17

We present measurements of the angular cross-correlation between luminous red galaxies from the Sloan Digital Sky Survey and the cosmic microwave background temperature maps from t…

astro-ph2003★ 134 cited

Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies

Tamas Budavari, Andrew J. Connolly, Alexander S. Szalay +18

Understanding the clustering of galaxies has long been a goal of modern observational cosmology. Utilizing our photometric redshift technique a volume limited sample containing mor…

astro-ph1999★ 71 cited

Reconstructing Galaxy Spectral Energy Distributions from Broadband Photometry

I. Csabai, A. J. Connolly, A. S. Szalay +1

We present a novel approach to photometric redshifts, one that merges the advantages of both the template fitting and empirical fitting algorithms, without any of their disadvantag…