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researcher

N. Seymour

131 papers hereh-index 457.9k citations241 works total

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

author position
  • first author1
  • middle author95
  • last author7

Across the 103 of 131 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO56
  • astro-ph.GA56
  • astro-ph14
  • astro-ph.IM4
  • astro-ph.HE1
same name
  • 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
  • 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
20012026
most citedThe Herschel Multi-tiered Extragalactic Survey: HerMES

800 citations · 7.5k across the 130 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 14 cited

Properties of X-ray selected Broad Absorption Line Quasars

A. J. Blustin, T. Dwelly, M. J. Page +6

Broad absorption line quasars (commonly termed BALQSOs) contain the most dramatic examples of AGN-driven winds. The high absorbing columns in these winds, ~10^24 cm^-2, ensure that…

astro-ph2008★ 30 cited

Mid-Infrared Spectra of High Redshift (z>2) Radio Galaxies

N. Seymour, P. Ogle, C. De Breuck +8

We present the first mid-infrared Spitzer/Infrared Spectrograph (IRS) observations of powerful radio galaxies at z>2. These radio galaxies, 4C +23.56 (z=2.48) and 6C J1908+7220 (z=…

astro-ph2008

The Contribution of Radio Selected Star Forming Galaxies to the IR Energy Density Budget

N. Seymour, T. Dwelly, D. Moss +6

We have used several different methods (radio morphology, radio spectral index, mid-IR to radio and near-IR to radio flux density ratios) to discriminate between AGN and SFGs in fa…

astro-ph2008★ 190 cited

The Star Formation History of the Universe as Revealed by Deep Radio Observations

N. Seymour, T. Dwelly, D. Moss +6

Discerning the exact nature of the sub-mJy radio population has been historically difficult due to the low luminosity of these sources at most wavelengths. Using deep ground based…

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