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researcher

N. Seymour

45 papers hereh-index 211.2k citations47 works total

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

author position
  • first author6
  • middle author24
  • last author3

Across the 33 of 45 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO23
  • astro-ph.GA13
  • astro-ph7
  • astro-ph.IM2
same name
  • N. Seymour — 131 papers, h 45
  • N. Seymour — 17 papers, h 3
  • N. Seymour — 10 papers, h 6
  • N. Seymour — 6 papers, h 3
  • N. Seymour — 6 papers, h 1
  • N. Seymour — 4 papers

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
20022026
most citedThe Herschel PEP/HerMES Luminosity Function. I: Probing the Evolution of PACS selected Galaxies to z~4

440 citations · 2.8k across the 45 of their papers we have counts for

collaborators
Showing 2017Show all

3 papers · 1 filter

astro-ph.CO2017★ 101 cited

OzDES multifibre spectroscopy for the Dark Energy Survey: Three year results and first data release

M. J. Childress, C. Lidman, T. M. Davis +98

We present results for the first three years of OzDES, a six-year programme to obtain redshifts for objects in the Dark Energy Survey (DES) supernova fields using the 2dF fibre pos…

astro-ph.GA2017★ 79 cited

Galaxy And Mass Assembly: The 1.4GHz SFR indicator, SFR-M* relation and predictions for ASKAP-GAMA

L. J. M. Davies, M. T. Huynh, A. M. Hopkins +20

We present a robust calibration of the 1.4GHz radio continuum star formation rate (SFR) using a combination of the Galaxy And Mass Assembly (GAMA) survey and the Faint Images of th…

astro-ph.GA2017★ 81 cited

The implications of the surprising existence of a large, massive CO disk in a distant protocluster

H. Dannerbauer, M. D. Lehnert, B. H. C. Emonts +18

It is not yet known if the properties of molecular gas in distant protocluster galaxies are significantly affected by their environment as galaxies are in local clusters. Through a…

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