activity
19932011
most citedContinuum and Emission Line Strength Relations for a large Active Galactic Nuclei Sample

185 citations · 614 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.CO2011★ 19 cited

LBQS 0103-2753: A Binary Quasar in a Major Merger

G. A. Shields, D. J. Rosario, V. Junkkarinen +3

We present HST and UKIRT spectra and images of the 2 kpc binary quasar LBQS 0103-2753 (z=0.858). The HST images (V- and I-band) show tidal features demonstrating that this system i…

astro-ph2006★ 11 cited

Hubble Space Telescope Ultraviolet Spectroscopy of Fourteen Low-Redshift Quasars

Rajib Ganguly, Michael S. Brotherton, Nahum Arav +35

We present low-resolution ultraviolet spectra of 14 low redshift (z<0.8) quasars observed with HST/STIS as part of a Snap project to understand the relationship between quasar outf…

astro-ph2004★ 21 cited

The Discovery of a High Redshift X-ray Emitting QSO Very Close to the Nucleus of NGC 7319

Pasquale Galianni, E. M. Burbidge, H. Arp +3

A strong X-ray source only 8" from the nucleus of the Sy2 galaxy NGC 7319 in Stephan's Quintet has been discovered by Chandra. We have identified the optical counterpart and show i…

astro-ph2004★ 120 cited

Dust and Diffuse Interstellar Bands in the z_a = 0.524 Absorption System toward AO 0235+164

V. T. Junkkarinen, Ross D. Cohen, E. A. Beaver +3

We present new HST STIS NUV-MAMA and STIS CCD observations of the BL Lac object AO 0235+164 and the intervening damped Ly alpha (DLA) line at z_a = 0.524. The line profile gives N(…

astro-ph2003★ 84 cited

Variability Tests for Intrinsic Absorption Lines in Quasar Spectra

Desika Narayanan, Fred Hamann, Tom Barlow +4

Quasar spectra have a variety of absorption lines whose origins range from energetic winds expelled from the central engines to unrelated, intergalactic clouds. We present multi-ep…

astro-ph2003★ 2 cited

How Massive Are BALQSO Winds?

F. Hamann, B. Sabra, V. Junkkarinen +2

We are involved in a program to derive properties of broad absorption line (BAL) winds in quasars using combined UV and X-ray observations. A major obstacle is large uncertainties…