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researcher

P. Monaco

108 papers hereh-index 425.6k citations149 works total

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

author position
  • sole author11
  • first author11
  • middle author53
  • last author12

Across the 87 of 108 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO50
  • astro-ph36
  • astro-ph.GA21
  • astro-ph.IM1
same name
  • P. Monaco — 147 papers, h 7
  • P. Monaco — 24 papers, h 15
  • P. Monaco — 10 papers, h 2
  • P. Monaco — 5 papers, h 3
  • P. Monaco — 3 papers, h 1
  • P. Monaco — 1 paper

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
19942026
most citedDifferent star formation laws for disks versus starbursts at low and high redshifts

741 citations · 6.5k across the 104 of their papers we have counts for

collaborators
Showing 2016 · astro-ph.GAShow all

3 papers · 2 filters

astro-ph.GA2016★ 8 cited

Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift z=0

David Goz, Pierluigi Monaco, Gian Luigi Granato +5

We present predictions of Spectral Energy Distributions (SEDs), from the UV to the FIR, of simulated galaxies at z=0. These were obtained by post-processing the results of an N-b…

astro-ph.GA2016★ 47 cited

The Formation of Supermassive Black Holes from Population III.1 Seeds. I. Cosmic Formation Histories and Clustering Properties

Nilanjan Banik, Jonathan C. Tan, Pierluigi Monaco

We calculate cosmic distributions in space and time of the formation sites of the first, "Pop III.1" stars, exploring a model in which these are the progenitors of all supermassive…

astro-ph.GA2016★ 60 cited

Kinetic AGN Feedback Effects on Cluster Cool Cores Simulated using SPH

Paramita Barai, Giuseppe Murante, Stefano Borgani +4

We implement novel numerical models of AGN feedback in the SPH code GADGET-3, where the energy from a supermassive black hole (BH) is coupled to the surrounding gas in the kinetic…

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