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P. Armitage

5 papers hereh-index 210 citations5 works total

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

author position
  • middle author3
  • last author2

Across the 5 of 5 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP2
  • astro-ph.CO1
  • astro-ph.HE1
  • astro-ph.SR1
same name
  • P. Armitage — 165 papers, h 57
  • P. Armitage — 9 papers, h 7
  • P. Armitage — 4 papers, h 38
  • P. Armitage — 3 papers, h 3
  • P. Armitage — 1 paper, h 7

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
20092026
most citedDBNets2.0: simulation-based inference for planet-induced dust substructures in protoplanetary discs

7 citations · 8 across the 5 of their papers we have counts for

collaborators
Showing 2025Show all

3 papers · 1 filter

astro-ph.HE2025

Pulsational Instability of Quasi-Stars: Interpreting the Variability of Little Red Dots

Matteo Cantiello, Jake B. Hassan, Rosalba Perna +5

The JWST discovery of "Little Red Dots" (LRDs) has revealed a population of compact, red sources at z∼5−10 that likely host supermassive black holes (SMBHs). Recent observat…

astro-ph.SR2025★ 1 cited

The Growth of the Central Black Holes in Quasi-stars

Jake Hassan, Rosalba Perna, Matteo Cantiello +3

Observations by JWST have confirmed the presence of supermassive black holes (BHs) at redshifts z≳10, lending support to scenarios in which BHs experience rapid growth thro…

astro-ph.EP2025★ 7 cited

DBNets2.0: simulation-based inference for planet-induced dust substructures in protoplanetary discs

A. Ruzza, G. Lodato, G. P. Rosotti +1

Dust substructures in protoplanetary discs can be signatures of embedded young planets whose detection and characterisation would provide a better understanding of planet formation…

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