papers

Publications (60)

astro-ph.GA2020

Significant Suppression of Star Formation in Radio-Quiet AGN Host Galaxies with Kiloparsec-Scale Radio Structures

Krista Lynne Smith, Michael Koss, Richard Mushotzky +4

We conducted 22~GHz 1" JVLA imaging of 100 radio-quiet X-ray selected AGN from the Swift-BAT survey. We find AGN-driven kiloparsec-scale radio structures inconsistent with pure sta…

astro-ph.GA2016

BAT AGN Spectroscopic Survey-III. An observed link between AGN Eddington ratio and narrow emission line ratios

Kyuseok Oh, Kevin Schawinski, Michael Koss +14

We investigate the observed relationship between black hole mass (), bolometric luminosity (), and Eddington ratio () with optical emission l…

astro-ph.GA2016

Active Galactic Nuclei from HeII: a more complete census of AGN in SDSS galaxies yields a new population of low-luminosity AGN in highly star-forming galaxies

Rudolf Bär, Anna K. Weigel, Lia F. Sartori +3

In order to perform a more complete census of active galactic nuclei (AGN) in the local Universe, we investigate the use of the HeII~ emission line diagnostic diagram by Sh…

astro-ph.HE2017

BAT AGN Spectroscopic Survey I: Spectral Measurements, Derived Quantities, and AGN Demographics

Michael Koss, Benny Trakhtenbrot, Claudio Ricci +20

We present the first catalog and data release of the Swift-BAT AGN Spectroscopic Survey (BASS). We analyze optical spectra of the majority of AGN (77%, 641/836) detected based on t…

astro-ph.GA2023

The Accretion History of AGN: The Spectral Energy Distributions of X-ray Luminous AGN

Connor Auge, David Sanders, Ezequiel Treister +17

Spectral energy distributions (SEDs) from X-ray to far-infrared (FIR) wavelengths are presented for a sample of 1246 X-ray luminous active galactic nuclei (AGN; $L_{0.5-10\rm{keV}}…

astro-ph.CO2011

Chandra Discovery of a Binary Active Galactic Nucleus in Mrk 739

Michael Koss, Richard Mushotzky, Ezequiel Treister +6

We have discovered a binary AGN in the galaxy Mrk 739 using Chandra and Swift BAT. We find two luminous L_2-10 keV=1.1*10^43 and 1.0*10^42 erg/s, unresolved nuclei with a projected…