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researcher

S. Walker

6 papers hereh-index 3149 citations8 works total

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

author position
  • middle author2
  • last author4

Across the 6 of 6 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph.HE3
same name
  • S. Walker — 58 papers, h 42
  • S. Walker — 39 papers, h 23
  • S. Walker — 36 papers, h 30
  • S. Walker — 23 papers, h 18
  • S. Walker — 19 papers, h 8
  • S. Walker — 18 papers, h 12

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
20232025
most citedA massive quiescent galaxy at redshift 4.658

232 citations · 235 across the 6 of their papers we have counts for

collaborators
Showing 2025Show all

4 papers · 1 filter

astro-ph.HE2025

From Observations to Simulations: A Neural-Network Approach to Intracluster Medium Kinematics

E. Gatuzz, J. ZuHone, J. S. Sanders +4

We present a systematic comparison between {\it XMM-Newton} velocity maps of the Virgo, Centaurus, Ophiuchus and A3266 clusters and synthetic velocity maps generated from the Illus…

astro-ph.HE2025★ 2 cited

The Quiescent Merging Nature of the Coma Cluster Revealed by ICM Velocity Structure

E. Gatuzz, J. Sanders, A. Liu +4

The hot gas permeating galaxy clusters-the intracluster medium (ICM)-is a key tracer of their assembly history and internal dynamics. Understanding the motion of this gas provides…

astro-ph.GA2025

Hidden (absorbed) Cooling Flows V: Groups and Galaxies including Spirals

A. C. Fabian, J. S. Sanders, G. J. Ferland +4

Cooling flows are observed in X-ray studies of the centres of cool core clusters, galaxy groups and individual elliptical galaxies. They are partly hidden from direct view by embed…

astro-ph.HE2025

Chemical enrichment of ICM within the A3266 cluster I: radial profiles

E. Gatuzz, J. Sanders, A. Liu +7

We present a detailed study of the elemental abundances distribution of the intracluster medium (ICM) within the A3266 cluster using {\it XMM-Newton} observations. This analysis us…

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