activity
20062026
most citedThe 105 month Swift-BAT all-sky hard X-ray survey

414 citations · 8.8k across the 184 of their papers we have counts for

collaborators
Showing 2016Show all

10 papers · 1 filter

astro-ph.GA2016★ 130 cited

ALMA Observations Show Major Mergers Among the Host Galaxies of Fast-growing, High-redshift Supermassive Black Holes

Benny Trakhtenbrot, Paulina Lira, Hagai Netzer +3

We present new ALMA band-7 data for a sample of six luminous quasars at z~4.8, powered by fast-growing supermassive black holes (SMBHs) with rather uniform properties: the typical…

astro-ph.GA2016★ 105 cited

The Complete Infrared View of Active Galactic Nuclei from the 70-month Swift/BAT Catalog

Kohei Ichikawa, Claudio Ricci, Yoshihiro Ueda +5

We systematically investigate the near- (NIR) to far-infrared (FIR) photometric properties of a nearly complete sample of local active galactic nuclei (AGN) detected in the Swift/B…

astro-ph.GA2016★ 120 cited

Optical variability of AGN in the PTF/iPTF survey

Neven Caplar, Simon J. Lilly, Benny Trakhtenbrot

We characterize the optical variability of quasars in the intermediate Palomar Transient Factory (iPTF) and Palomar Transient Factory (PTF) surveys. We re-calibrate the -band li…

astro-ph.GA2016★ 64 cited

On the Accretion Rates and Radiative Efficiencies of the Highest Redshift Quasars

Benny Trakhtenbrot, Marta Volonteri, Priyamvada Natarajan

We estimate the accretion rates onto the supermassive black holes that power 20 of the highest-redshift quasars, at z>5.8, including the quasar with the highest redshift known to d…

astro-ph.GA2016★ 30 cited

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 li…

astro-ph.GA2016★ 25 cited

The Chandra COSMOS Legacy Survey: Clustering of X-ray selected AGN at 2.9<z<5.5 using photometric redshift Probability Distribution Functions

V. Allevato, F. Civano, A. Finoguenov +16

We present the measurement of the projected and redshift space 2-point correlation function (2pcf) of the new catalog of Chandra COSMOS-Legacy AGN at 2.9z5.5 ($\langle…

astro-ph.GA2016★ 9 cited

Testing the Completeness of the SDSS Colour Selection for Ultramassive, Slowly Spinning Black Holes

Caroline Bertemes, Benny Trakhtenbrot, Kevin Schawinski +2

We investigate the sensitivity of the colour-based quasar selection algorithm of the Sloan Digital Sky Survey to several key physical parameters of supermassive black holes (SMBHs)…

astro-ph.GA2016★ 28 cited

Determining the radio AGN contribution to the radio-FIR correlation using the black hole fundamental plane relation

O. Ivy Wong, M. J. Koss, K. Schawinski +5

We investigate the 1.4 GHz radio properties of 92 nearby (z<0.05) ultra hard X-ray selected Active Galactic Nuclei (AGN) from the Swift Burst Alert Telescope (BAT) sample. Through…

astro-ph.GA2016★ 57 cited

Active galactic nuclei at z ~ 1.5: III. Accretion discs and black hole spin

Daniel M. Capellupo, Hagai Netzer, Paulina Lira +2

This is the third paper in a series describing the spectroscopic properties of a sample of 39 AGN at , selected to cover a large range in black hole mass () and…

astro-ph.GA2016★ 147 cited

Active galactic nuclei at z~1.5: II. Black Hole Mass estimation by means of broad emission lines

Julián E. Mejía-Restrepo, Benny Trakhtenbrot, Paulina Lira +2

This is the second in a series of papers aiming to test how the mass (), accretion rate () and spin () of super massive black holes (SMBHs) determine th…