activity
20102026
most citedThe Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

1.9k citations · 9k across the 138 of their papers we have counts for

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Showing 2017Show all

16 papers · 1 filter

astro-ph.GA2017★ 19 cited

Joint NuSTAR and Chandra analysis of the obscured quasar in IC 2497 - Hanny's Voorwerp system

Lia F. Sartori, Kevin Schawinski, Michael J. Koss +9

We present new Nuclear Spectroscopic Telescope Array (NuSTAR) observations of the core of IC 2497, the galaxy associated with Hanny's Voorwerp. The combined fits of the Chandra (0.…

astro-ph.GA2017★ 36 cited

BAT AGN Spectroscopic Survey--VIII. Type 1 AGN With Massive Absorbing Columns

T. Taro Shimizu, Richard I. Davies, Michael Koss +12

We explore the relationship between X-ray absorption and optical obscuration within the BAT AGN Spectroscopic Survey (BASS) which has been collecting and analyzing the optical and…

astro-ph.GA2017★ 83 cited

LLAMA: Normal star formation efficiencies of molecular gas in the centres of luminous Seyfert galaxies

D. J. Rosario, L. Burtscher, R. I. Davies +23

Using new APEX and JCMT spectroscopy of the CO 2-1 line, we undertake a controlled study of cold molecular gas in moderately luminous Active Galactic Nuclei (AGN) and inactive gala…

astro-ph.GA2017★ 16 cited

LLAMA: Nuclear stellar properties of Swift BAT AGN and matched inactive galaxies

Ming-Yi Lin, R. I. Davies, E. K. S. Hicks +20

In a complete sample of local 14-195 keV selected AGNs and inactive galaxies, matched by their host galaxy properties, we study the spatially resolved stellar kinematics and lumino…

astro-ph.GA2017★ 10 cited

Investigating the evolution of the dual AGN system ESO~509-IG066

P. Kosec, M. Brightman, D. Stern +13

We analyze the evolution of the dual AGN in ESO 509-IG066, a galaxy pair located at z=0.034 whose nuclei are separated by 11 kpc. Previous observations with XMM-Newton on this dual…

astro-ph.HE2017★ 332 cited

The close environments of accreting massive black holes are shaped by radiative feedback

Claudio Ricci, Benny Trakhtenbrot, Michael J. Koss +13

The large majority of the accreting supermassive black holes in the Universe are obscured by large columns of gas and dust. The location and evolution of this obscuring material ha…