activity
20172022
most citedThe Field Substellar Mass Function Based on the Full-sky 20-pc Census of 525 L, T, and Y Dwarfs

171 citations · 887 across the 14 of their papers we have counts for

collaborators
Showing 2019Show all

6 papers · 1 filter

astro-ph.HE2019★ 5 cited

The Broadband X-ray Spectrum of the X-ray Obscured Type 1 AGN 2MASX J193013.80+341049.5

Nikita Kamraj, Mislav Baloković, Murray Brightman +6

We present results from modeling the broadband X-ray spectrum of the Type 1 AGN 2MASX J193013.80+341049.5 using NuSTAR, Swift and archival XMM-Newton observations. We find this sou…

astro-ph.GA2019★ 38 cited

The Spectral Energy Distributions of Active Galactic Nuclei

M. J. I. Brown, K. J. Duncan, H. Landt +5

We present spectral energy distributions (SEDs) of 41 active galactic nuclei, derived from multiwavelength photometry and archival spectroscopy. All of the SEDs span at least 0.09…

astro-ph.HE2019

Probing the Black Hole Engine with Measurements of the Relativistic X-ray Reflection Component

Javier A. García, Matteo Bachetti, David R. Ballantyne +21

Over the last decades X-ray spectroscopy has proven to be a powerful tool for the estimation of black hole spin and several other key parameters in dozens of AGN and black hole X-r…

astro-ph.HE2019★ 3 cited

Probing the Physical Properties of the Corona in Accreting Black Holes

Nikita Kamraj, Andrew Fabian, Anne Lohfink +3

The corona is a key component of most luminous accreting black holes, carrying 5 - 30 % of the power and in non-jetted Active Galactic Nuclei (AGN), creating all the X-ray emission…

astro-ph.GA2019★ 38 cited

The Spectral Energy Distributions of Active Galactic Nuclei

M. J. I. Brown, K. J. Duncan, H. Landt +3

We present ongoing work on the spectral energy distributions (SEDs) of active galactic nuclei (AGNs), derived from X-ray, ultraviolet, optical, infrared and radio photometry and sp…

astro-ph.GA2019★ 108 cited

A new class of flares from accreting supermassive black holes

Benny Trakhtenbrot, Iair Arcavi, Claudio Ricci +26

Accreting supermassive black holes (SMBHs) can exhibit variable emission across the electromagnetic spectrum and over a broad range of timescales. The variability of active galacti…