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researcher

P. Tozzi

57 papers hereh-index 282.6k citations57 works total

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

author position
  • first author1
  • middle author33
  • last author10

Across the 44 of 57 papers where every author was matched, so the position is known.

fields
  • astro-ph25
  • astro-ph.GA14
  • astro-ph.CO13
  • astro-ph.IM3
  • astro-ph.HE2
same name
  • P. Tozzi — 171 papers, h 54
  • P. Tozzi — 5 papers, h 2
  • P. Tozzi — 5 papers, h 5
  • P. Tozzi — 4 papers, h 2
  • P. Tozzi — 2 papers
  • P. Tozzi — 2 papers, h 4

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19972026
most citedX-ray spectral properties of AGN in the Chandra Deep Field South

388 citations · 4k across the 57 of their papers we have counts for

collaborators
Showing 2006Show all

4 papers · 1 filter

astro-ph2006

Tracing the evolution in the iron content of the ICM

I. Balestra, P. Tozzi, S. Ettori +4

We present a Chandra analysis of the X-ray spectra of 56 clusters of galaxies at z>0.3, which cover a temperature range of 3>kT>15 keV. Our analysis is aimed at measuring the iron…

astro-ph2006★ 151 cited

Tracing the evolution in the iron content of the ICM

I. Balestra, P. Tozzi, S. Ettori +5

We present a Chandra analysis of the X-ray spectra of 56 clusters of galaxies at z>0.3, which cover a temperature range 3<kT<15 keV. Our analysis is aimed at measuring the iron abu…

astro-ph2006★ 388 cited

X-ray spectral properties of AGN in the Chandra Deep Field South

P. Tozzi, R. Gilli, V. Mainieri +12

We present a detailed X-ray spectral analysis of the sources in the 1Ms catalog of the Chandra Deep Field South (CDFS) taking advantage of optical spectroscopy and photometric reds…

astro-ph2006

AGN and Galaxy evolution from Deep X-ray surveys

P. Tozzi, R. Gilli, the CDFS Team

Deep X-ray surveys are providing crucial information on the evolution of AGN and galaxies. We review some of the latest results based on the X-ray spectral analysis of the sources…

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