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researcher

N. Seymour

4 papers hereh-index 2184 citations3 works total

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

author position
  • middle author3

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
  • astro-ph1
same name
  • N. Seymour — 131 papers, h 45
  • N. Seymour — 45 papers, h 21
  • N. Seymour — 17 papers, h 3
  • N. Seymour — 10 papers, h 6
  • N. Seymour — 6 papers, h 3
  • N. Seymour — 6 papers, h 1

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
20082025
most citedThe type IIb SN 2008ax: spectral and light curve evolution

146 citations · 288 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.GA2025

The Centre of Attention: a Powerful Radio Galaxy Pinpoints a NIR-Dark Protocluster at z~3.9

A. J. Hedge, N. Seymour, J. W. Broderick +8

We report the discovery of a z∼3.9 protocluster identified from Atacama Large Millimetre/sub-millimetre Array Band 3 spectral scans of a bright radio source selected from the…

astro-ph.GA2015★ 36 cited

The formation history of massive cluster galaxies as revealed by CARLA

E. A. Cooke, N. A. Hatch, A. Rettura +12

We use a sample of 37 of the densest clusters and protoclusters across 1.3≤z≤3.2 from the Clusters Around Radio-Loud AGN (CARLA) survey to study the formation of massive…

astro-ph.GA2014★ 106 cited

Why z > 1 radio-loud galaxies are commonly located in proto-clusters

N. A. Hatch, D. Wylezalek, J. D. Kurk +9

Distant powerful radio-loud active galactic nuclei (RLAGN) tend to reside in dense environments and are commonly found in proto-clusters at z > 1.3. We examine whether this occurs…

astro-ph2008★ 146 cited

The type IIb SN 2008ax: spectral and light curve evolution

A. Pastorello, M. M. Kasliwal, R. M. Crockett +12

We present spectroscopy and photometry of the He-rich supernova (SN) 2008ax. The early-time spectra show prominent P-Cygni H lines, which decrease with time and disappear completel…

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