activity
20082020
most citedTurbulent Heating in Galaxy Clusters Brightest in X-rays

340 citations · 1.7k across the 25 of their papers we have counts for

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Showing 2015Show all

7 papers · 1 filter

astro-ph.HE2015★ 58 cited

The NuSTAR view of reflection and absorption in NGC 7582

E. Rivers, M. Baloković, P. Arévalo +14

NGC 7582 is a well-studied X-ray bright Seyfert 2 with moderately heavy (~cm), highly variable absorption and strong reflection spectral fea…

astro-ph.HE2015★ 52 cited

The hard X-ray emission of the luminous infrared galaxy NGC 6240 as observed by NuSTAR

S. Puccetti, A. Comastri, F. E. Bauer +23

We present a broad-band (~0.3-70 keV) spectral and temporal analysis of NuSTAR observations of the luminous infrared galaxy NGC 6240, combined with archival Chandra, XMM-Newton and…

astro-ph.HE2015★ 66 cited

NuSTAR Observations of the Compton-thick Active Galactic Nucleus and Ultraluminous X-ray Source Candidate in NGC 5643

A. Annuar, P. Gandhi, D. M. Alexander +22

We present two NuSTAR observations of the local Seyfert 2 active galactic nucleus (AGN) and an ultraluminous X-ray source (ULX) candidate in NGC 5643. Together with archival data f…

astro-ph.GA2015★ 41 cited

On the Nature of X-ray Surface Brightness Fluctuations in M87

P. Arévalo, E. Churazov, I. Zhuravleva +2

X-ray images of galaxy clusters and gas-rich elliptical galaxies show a wealth of small-scale features which reflect fluctuations in density and/or temperature of the intra-cluster…

astro-ph.GA2015★ 27 cited

The QUEST-La Silla AGN Variability Survey

Régis Cartier, Paulina Lira, Paolo Coppi +7

We present the characterization and initial results from the QUEST-La Silla AGN variability survey. This is an effort to obtain well sampled optical light curves in extragalactic f…

astro-ph.HE2015

The NuSTAR X-ray spectrum of the low-luminosity AGN in NGC 7213

F. Ursini, A. Marinucci, G. Matt +11

We present an analysis of the 3-79 keV NuSTAR spectrum of the low-luminosity active galactic nucleus NGC 7213. In agreement with past observations, we find a lower limit to the hig…