activity
20082011
most citedA Search for Binary Active Galactic Nuclei: Double-Peaked [OIII] AGN in the Sloan Digital Sky Survey

201 citations · 347 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO2011

Double-Peaked Narrow Emission Lines in AGN: The Role of Rotating Disks

Krista Lynne Smith, G. A. Shields, S. Salviander +2

AGN with double-peaked narrow lines (DPAGN) may be caused by kiloparsec scale binary AGN, bipolar outflows, or rotating gaseous disks. We examine the class of DPAGN in which the tw…

astro-ph.CO2010★ 23 cited

The Nuclear Outflow in NGC 2110

D. J. Rosario, M. Whittle, C. H. Nelson +1

We present a HST/STIS spectroscopic and optical/radio imaging study of the Seyfert NGC 2110 aiming to measure the dynamics and understand the nature of the nuclear outflow in the g…

astro-ph.HE2010★ 16 cited

The Radio Jet Interaction in NGC 5929: Direct Detection of Shocked Gas

D. J. Rosario, M. Whittle, C. H. Nelson +1

We report the discovery of kinematic shock signatures associated with a localized radio jet interaction in the merging Seyfert galaxy NGC 5929. We explore the velocity-dependent io…

astro-ph.CO2009★ 201 cited

A Search for Binary Active Galactic Nuclei: Double-Peaked [OIII] AGN in the Sloan Digital Sky Survey

Krista L. Smith, G. A. Shields, E. W. Bonning +3

We present AGN from the Sloan Digital Sky Survey (SDSS) having double-peaked profiles of [OIII] 5007,4959 and other narrow emission-lines, motivated by the prospect of finding cand…

astro-ph.CO2009★ 72 cited

The Quasar SDSS J105041.35+345631.3: Black Hole Recoil or Extreme Double-Peaked Emitter?

G. A. Shields, D. J. Rosario, K. L. Smith +8

The quasar SDSS J105041.35+345631.3 (z = 0.272) has broad emission lines blueshifted by 3500 km/s relative to the narrow lines and the host galaxy. Such an object may be a candidat…

astro-ph2008★ 35 cited

AEGIS: Radio and Mid-Infrared Selection of Obscured AGN Candidates

S. Q. Park, P. Barmby, G. G. Fazio +10

The application of multi-wavelength selection techniques is crucial for discovering a complete and unbiased set of Active Galactic Nuclei (AGNs). Here, we select a sample of 72 AGN…