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researcher

D. Nelson

4 papers hereh-index 446 citations5 works total

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

author position
  • middle author1

Across the 1 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA2
  • astro-ph.CO1
  • astro-ph.HE1
same name
  • D. Nelson — 14 papers, h 59
  • D. Nelson — 5 papers, h 1
  • D. Nelson — 3 papers, h 3
  • D. Nelson — 1 paper, h 6

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

collaborators

4 papers

astro-ph.GA2025

Exploring the statistical properties of double radio relics in the TNG-Cluster and TNG300 simulations

Wonki Lee, Annalisa Pillepich, Dylan Nelson +4

Double radio relics, pairs of diffuse radio features located on opposite sides of merging galaxy clusters, are a rare subclass of radio relics that are believed to trace merger sho…

astro-ph.GA2025

Comparing XRISM cluster velocity dispersions with predictions from cosmological simulations: are feedback models too ejective?

XRISM Collaboration, Marc Audard, Hisamitsu Awaki +147

The dynamics of the intra-cluster medium (ICM), the hot plasma that fills galaxy clusters, are shaped by gravity-driven cluster mergers and feedback from supermassive black holes (…

astro-ph.CO2025

Atacama Large Aperture Submillimeter Telescope (AtLAST) Science: Resolving the Hot and Ionized Universe through the Sunyaev-Zeldovich effect

Luca Di Mascolo, Yvette Perrott, Tony Mroczkowski +23

An omnipresent feature of the multi-phase ``cosmic web'' is that warm/hot (>105 K) ionized gas pervades it. This gas constitutes a relevant contribution to the overall universal…

astro-ph.HE2025

XRISM forecast for the Coma cluster: stormy, with a steep power spectrum

XRISM Collaboration, Marc Audard, Hisamitsu Awaki +142

The XRISM Resolve microcalorimeter array measured the velocities of hot intracluster gas at two positions in the Coma galaxy cluster: 3'x3' squares at the center and at 6' (170 kpc…

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