activity
19952020
most citedProbing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts

418 citations · 1.8k across the 34 of their papers we have counts for

collaborators

33 papers

cs.CL2020★ 3 cited

Quantification of BERT Diagnosis Generalizability Across Medical Specialties Using Semantic Dataset Distance

Mihir P. Khambete, William Su, Juan Garcia +1

Deep learning models in healthcare may fail to generalize on data from unseen corpora. Additionally, no quantitative metric exists to tell how existing models will perform on new d…

astro-ph2006★ 418 cited

Probing the Coevolution of Supermassive Black Holes and Galaxies Using Gravitationally Lensed Quasar Hosts

C. Y. Peng, C. D. Impey, H. -W. Rix +5

In the present-day universe, supermassive black hole masses (MBH) appear to be strongly correlated with their galaxy's bulge luminosity, among other properties. In this study, we e…

astro-ph2006★ 13 cited

Lensed Quasar Hosts

Chien Y. Peng, Chris D. Impey, Hans-Walter Rix +5

Gravitational lensing assists in the detection of quasar hosts by amplifying and distorting the host light away from the unresolved quasar core images. We present the results of HS…

astro-ph2005★ 62 cited

First Results from a Photometric Survey of Strong Gravitational Lens Environments

K. A. Williams, I. Momcheva, C. R. Keeton +2

Many strong gravitational lenses lie in complex environments, such as poor groups of galaxies, that significantly bias conclusions from lens analyses. We are undertaking a photomet…

astro-ph2005★ 11 cited

The FIRST-Optical-VLA Survey for Lensed Radio Lobes

D. B. Haarsma, J. N. Winn, E. E. Falco +7

We present results from a survey for gravitationally lensed radio lobes. Lensed lobes are a potentially richer source of information about galaxy mass distributions than lensed poi…

astro-ph2004★ 128 cited

Radio Variability of Radio Quiet and Radio Loud Quasars

Richard Barvainis, Joseph Lehar, Mark Birkinshaw +2

The majority of quasars are weak in their radio emission, with flux densities comparable to those in the optical, and energies far lower. A small fraction, about 10%, are hundreds…