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P. Tozzi

4 papers hereh-index 225 citations6 works total

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

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO2
  • astro-ph.GA2
same name
  • P. Tozzi — 171 papers, h 54
  • P. Tozzi — 57 papers, h 28
  • P. Tozzi — 5 papers, h 2
  • P. Tozzi — 5 papers, h 5
  • 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
20162025
most citedCHEX-MATE: Characterization of the intra-cluster medium temperature distribution

22 citations · 45 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2025

Understanding entropy in massive halos: The role of baryon decoupling

S. Molendi, M. Balboni, I. Bartalucci +8

The goal of the work presented in this paper is to use observed entropy profiles to infer constraints on the accretion process in massive halos. We compare entropy profiles from va…

astro-ph.CO2024★ 3 cited

Cooling rate and turbulence in the intracluster medium of the cool-core cluster Abell 2667

M. Lepore, C. Pinto, P. Tozzi +8

We present a detailed analysis of the thermal X-ray emission from the intracluster medium (ICM) in the cool-core galaxy cluster Abell 2667 (z=0.23). Our goal is to detect low-tem…

astro-ph.CO2023★ 22 cited

CHEX-MATE: Characterization of the intra-cluster medium temperature distribution

L. Lovisari, S. Ettori, E. Rasia +23

We study the perturbations in the temperature (and density) distribution for 28 clusters selected from the CHEX-MATE sample to evaluate and characterize the level of inhomogeneitie…

astro-ph.GA2016★ 20 cited

Where does the gas fueling star formation in BCGs originate?

S. Molendi, P. Tozzi, M. Gaspari +4

We investigate the relationship between X-ray cooling and star formation in brightest cluster galaxies (BCGs). We present an X-ray spectral analysis of the inner regions, 10-40 kpc…

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