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researcher

M. Gray

4 papers hereh-index 5162 citations13 works total

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

author position
  • middle author3
  • last author1

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

fields
  • astro-ph.GA3
  • astro-ph.CO1
same name
  • M. Gray — 35 papers, h 28
  • M. Gray — 19 papers, h 27
  • M. Gray — 10 papers, h 32
  • M. Gray — 8 papers
  • M. Gray — 7 papers, h 7
  • M. Gray — 3 papers, h 2

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
20242026
most citedThe effect of cosmic web filaments on galaxy evolution

33 citations · 33 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2026

Enabling Cosmic Web Analysis at Gigaparsec Scales: A Multi Block Approach for DisPerSE

Ankit Singh, Frazer Pearce, Meghan Gray +1

Cosmic filaments are the longest structures in the Universe and the dominant element of the cosmic web, channelling matter onto clusters and shaping the environments in which galax…

astro-ph.CO2026

Searching for signatures of fuzzy dark matter in cosmic filament profiles

Callum J. O'Kane, Alfonso Aragón-Salamanca, Ulrike Kuchner +1

Current observations reveal persistent tensions with the standard cold dark matter paradigm, raising the question of whether these can be explained by baryonic physics alone or req…

astro-ph.GA2025

The life and times of dark matter haloes: what will I be when I grow up?

Julian Onions, Frazer Pearce, Alexander Knebe +6

Are the most massive objects in the Universe today the direct descendants of the most massive objects at higher redshift? We address this question by tracing the evolutionary histo…

astro-ph.GA2024★ 33 cited

The effect of cosmic web filaments on galaxy evolution

Callum J. O'Kane, Ulrike Kuchner, Meghan E. Gray +1

Galaxy properties are known to be affected by their environment. This is well established for the extremes of the density scales, between the high-density cluster environment and t…

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