activity
19962021
most citedReverberation Mapping of Optical Emission Lines in Five Active Galaxies

112 citations · 352 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2021★ 6 cited

AGN STORM 2: I. First results: A Change in the Weather of Mrk 817

Erin Kara, Missagh Mehdipour, Gerard A. Kriss +69

We present the first results from the ongoing, intensive, multi-wavelength monitoring program of the luminous Seyfert 1 galaxy Mrk 817. While this AGN was, in part, selected for it…

astro-ph.GA2016★ 112 cited

Reverberation Mapping of Optical Emission Lines in Five Active Galaxies

M. M. Fausnaugh, C. J. Grier, M. C. Bentz +68

We present the first results from an optical reverberation mapping campaign executed in 2014, targeting the active galactic nuclei (AGN) MCG+08-11-011, NGC 2617, NGC 4051, 3C 382,…

astro-ph.GA2013★ 6 cited

The story of Seyfert galaxy RE J2248-511: from intriguingly ultrasoft to unremarkably average

Rhaana Starling, C. Done, C. Jin +7

RE J2248-511 is one of only 14 non-blazar AGN detected in the far ultraviolet by the ROSAT Wide Field Camera implying a large ultrasoft X-ray flux. This soft X-ray excess is strong…

astro-ph2008★ 34 cited

Determining the extragalactic extinction law with SALT

Ido Finkelman, Noah Brosch, Alexei Y. Kniazev +7

We present CCD imaging observations of early-type galaxies with dark lanes obtained with the Southern African Large Telescope (SALT) during its performance-verification phase. We d…

astro-ph2007★ 37 cited

Adaptive optics imaging and optical spectroscopy of a multiple merger in a luminous infrared galaxy

P. Vaisanen, S. Mattila, A. Kniazev +16

(abridged) We present near-infrared (NIR) adaptive optics imaging obtained with VLT/NACO and optical spectroscopy from the Southern African Large Telescope (SALT) of a luminous inf…

astro-ph2004

The soft X-ray excess AGN RE J2248-511

R. L. C. Starling, E. M. Puchnarewicz, E. Romero-Colmenero

We model the spectral energy distribution of the ultrasoft broad-line AGN RE J2248-511 with Comptonised accretion disc models. These are able to reproduce the steep optical and ult…