activity
20042008
most citedNGC 5548: The AGN Energy Budget Problem and the Geometry of the Broad-Line Region and Torus

36 citations · 72 across the 8 of their papers we have counts for

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astro-ph20081 cited

How Polarization and Scattering can reveal Geometries, Dynamics, and Feeding of Active Galactic Nuclei

R. W. Goosmann, C. M. Gaskell, M. Shoji

Gaskell et al. (2007) introduced polarization reverberation mapping as a new technique to explore the structure of active galactic nuclei. We present modeling results for the time-…

astro-ph200736 cited

NGC 5548: The AGN Energy Budget Problem and the Geometry of the Broad-Line Region and Torus

C. Martin Gaskell, Elizabeth S. Klimek, Ludmila S. Nazarova

We consider in detail the spectral energy distribution (SED) and multi-wavelength variability of NGC5548. Comparison with the SEDs of other AGNs implies that the internal reddening…

astro-ph200730 cited

AGN Reddening and Ultraviolet Extinction Curves from Hubble Space Telescope Spectra

C. Martin Gaskell, A. J. Benker

We present intrinsic extinction curves for 14 AGNs. The AGNs have reddenings, E(B-V), of up to 0.36 mag. The majority (13 out of 14) of the extinction curves are not steep in the U…

astro-ph2007

Modeling the Polarization of Dusty Scattering Cones in Active Galactic Nuclei

Rene W. Goosmann, C. Martin Gaskell, M. Shoji

We have used the STOKES radiative transfer code, to model polarization induced by dust scattering in the polar regions of Active Galactic Nuclei (AGN). We discuss the wavelength-de…

astro-ph20063 cited

Optical and X-ray Variability of AGNs

C. Martin Gaskell

I present new comparisons of AGN optical, UV, and X-ray variations. These reveal complex relationships between the different passbands that can change with time in a given object.…

astro-ph2006

Optical Variability of the Three Brightest Nearby Quasars

C. Martin Gaskell, Andrew J. Benker, Jeffrey S. Campbell +9

We report on the relative optical variability of the three brightest nearby quasars, 3C 273, PDS 456, and PHL 1811. All three have comparable absolute magnitudes, but PDS 456 and P…