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researcher

Alberto Masini

3 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author3

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.GA1
ORCID 0000-0002-7100-9366

identity via Semantic Scholar / OpenAlex

most citedA growth-rate indicator for Compton-thick active galactic nuclei

37 citations · 66 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2019★ 1 cited

Resolving the cosmic X-ray background with a next-generation high-energy X-ray observatory

R. C. Hickox, F. Civano, D. R. Ballantyne +16

The cosmic X-ray background (CXB), which peaks at an energy of ~30 keV, is produced primarily by emission from accreting supermassive black holes (SMBHs). The CXB therefore serves…

astro-ph.GA2016★ 28 cited

IC 3639 - A new bona fide Compton thick AGN unveiled by NuSTAR

Peter G. Boorman, P. Gandhi, D. Alexander +19

We analyse high-quality NuSTAR observations of the local (z = 0.011) Seyfert 2 active galactic nucleus (AGN) IC 3639, in conjunction with archival Suzaku and Chandra data. This pro…

astro-ph.HE2016★ 37 cited

A growth-rate indicator for Compton-thick active galactic nuclei

M. Brightman, A. Masini, D. R. Ballantyne +10

Due to their heavily obscured central engines, the growth rate of Compton-thick (CT) active galactic nuclei (AGN) is difficult to measure. A statistically significant correlation b…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.