activity
20042017
most citedMid-Infrared Selection of Active Galaxies

936 citations · 1.6k across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2017★ 34 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IX: The Ninth Year (2016-2017)

Taichi Kato, Keisuke Isogai, Franz-Josef Hambsch +76

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016--201…

astro-ph.HE2017★ 62 cited

The ASAS-SN Bright Supernova Catalog -- III. 2016

T. W. -S. Holoien, J. S. Brown, K. Z. Stanek +36

This catalog summarizes information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) and all other bright (), spectroscopicall…

astro-ph.GA2009★ 513 cited

Host galaxies, clustering, Eddington ratios, and evolution of radio, X-ray, and infrared-selected AGNs

Ryan C. Hickox, Christine Jones, William R. Forman +15

We explore the connection between different classes of active galactic nuclei (AGNs) and the evolution of their host galaxies, by deriving host galaxy properties, clustering, and E…

astro-ph2008★ 22 cited

The Origin of the 24-micron Excess in Red Galaxies

Kate Brand, John Moustakas, Lee Armus +11

Observations with the Spitzer Space Telescope have revealed a population of red-sequence galaxies with a significant excess in their 24-micron emission compared to what is expected…

astro-ph2005★ 48 cited

Halo Structures of Gravitational Lens Galaxies

Jaiyul Yoo, Christopher S. Kochanek, Emilio E. Falco +1

We explore the halo structure of four gravitational lenses with well-observed, thin Einstein rings. We find that the gravitational potentials are well described by ellipsoidal dens…

astro-ph2005★ 34 cited

The Lens Galaxy In PG1115+080 is an Ellipse

Jaiyul Yoo, Christopher S. Kochanek, Emilio E. Falco +1

We use the structure of the Einstein ring image of the quasar host galaxy in the four-image quasar lens PG1115+080 to determine the angular structure of the gravitational potential…