activity
19952023
most citedThe Quiescent Intracluster Medium in the Core of the Perseus Cluster

500 citations · 2.7k across the 43 of their papers we have counts for

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Showing astro-ph.HEShow all

33 papers · 1 filter

astro-ph.HE2022

BASS XXX: Distribution Functions of DR2 Eddington-ratios, Black Hole Masses, and X-ray Luminosities

Tonima Tasnim Ananna, Anna K. Weigel, Benny Trakhtenbrot +19

We determine the low-redshift X-ray luminosity function (XLF), active black hole mass function (BHMF), and Eddington-ratio distribution function (ERDF) for both unobscured (Type 1)…

astro-ph.HE2021★ 10 cited

Probing the circumnuclear environment of NGC1275 with High-Resolution X-ray spectroscopy

Christopher S. Reynolds, Robyn N. Smith, Andrew C. Fabian +6

NGC1275 is the Brightest Cluster Galaxy (BCG) in the Perseus cluster and hosts the active galactic nucleus (AGN) that is heating the central 100\,kpc of the intracluster medium (IC…

astro-ph.HE2020

Forward Modeling Populations of Flares from Tidal Disruptions of Stars by Super-massive Black Holes

Nathaniel Roth, Sjoert van Velzen, S. Bradley Cenko +1

Detections of the tidal disruption flares (TDFs) of stars by supermassive black holes (SMBHs) are rapidly accumulating as optical surveys improve. These detections may provide cons…

astro-ph.HE2019

The BAT AGN Spectroscopic Survey -- XVIII. Searching for Supermassive Black Hole Binaries in the X-rays

Tingting Liu, Michael Koss, Laura Blecha +15

Theory predicts that a supermassive black hole binary (SMBHB) could be observed as a luminous active galactic nucleus (AGN) that periodically varies on the order of its orbital tim…

astro-ph.HE2019★ 11 cited

The nature of the broadband X-ray variability in the dwarf Seyfert galaxy NGC 4395

E. S. Kammoun, E. Nardini, A. Zoghbi +14

We present a flux-resolved X-ray analysis of the dwarf Seyfert 1.8 galaxy NGC 4395, based on three archival and one archival observations. The source is known…

astro-ph.HE2019

X-Ray Spectrum of RBS 315: Absorption or Intrinsic Curvature

Sivan Ben Haim, Ehud Behar, Richard F. Mushotzky

X-ray absorption of high-redshift quasars is enigmatic, because it remains unclear where in the universe the absorbing gas is. If absorption occurs near the high-z host, it could h…