activity
20012023
most citedNuSTAR catches the unveiling nucleus of NGC 1068

138 citations · 316 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.HE2023★ 3 cited

The High Energy X-ray Probe (HEX-P): Constraining Supermassive Black Hole Growth with Population Spin Measurements

J. M. Piotrowska, J. A. García, D. J. Walton +24

Constraining the primary growth channel of supermassive black holes (SMBH) remains one the most actively debated questions in the context of cosmological structure formation. Owing…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe (HEX-P): Probing the physics of the X-ray corona in active galactic nuclei

E. Kammoun, A. M. Lohfink, M. Masterson +28

The hard X-ray emission in active galactic nuclei (AGN) and black hole X-ray binaries is thought to be produced by a hot cloud of electrons referred to as the corona. This emission…

astro-ph.HE2015★ 138 cited

NuSTAR catches the unveiling nucleus of NGC 1068

A. Marinucci, S. Bianchi, G. Matt +15

We present a NuSTAR and XMM-Newton monitoring campaign in 2014/2015 of the Compton-thick Seyfert 2 galaxy, NGC 1068. During the August 2014 observation, we detect with NuSTAR a flu…

astro-ph.HE2014★ 35 cited

The Seyfert 2 galaxy NGC 2110: hard X-ray emission observed by NuSTAR and variability of the iron K line

A. Marinucci, G. Matt, S. Bianchi +16

We present NuSTAR observations of the bright Seyfert 2 galaxy NGC 2110 obtained in 2012, when the source was at the highest flux level ever observed, and in 2013, when the source w…

astro-ph.CO2010★ 31 cited

A characterization of the NGC 4051 soft X-ray spectrum as observed by XMM-Newton

A. A. Nucita, M. Guainazzi, A. L. Longinotti +3

Soft X-rays high resolution spectroscopy of obscured AGNs shows the existence of a complex soft -ray spectrum dominated by emission lines of He and H-like transitions of element…

astro-ph.CO2009★ 39 cited

AGN/starburst connection in action: the half million second RGS spectrum of NGC1365

M. Guainazzi, G. Risaliti, A. Nucita +4

We present a deep (~5.8 days) 0.3-2 keV high-resolution spectrum of NGC1365, collected with the reflection grating spectrometer (RGS) on board XMM-Newton. The spectrum is dominated…