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researcher

N. Evans

111 papers hereh-index 6514.1k citations310 works total

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

author position
  • sole author2
  • first author9
  • middle author33
  • last author34

Across the 78 of 111 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA51
  • astro-ph50
  • astro-ph.SR7
  • astro-ph.CO1
  • astro-ph.IM1
  • nlin.SI1
same name
  • N. Evans — 43 papers, h 55
  • N. Evans — 39 papers, h 32
  • N. Evans — 34 papers, h 23
  • N. Evans — 34 papers, h 53
  • N. Evans — 9 papers, h 16
  • N. Evans — 7 papers, h 14

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
19982022
most citedBeasts of the Southern Wild: Discovery of nine Ultra Faint satellites in the vicinity of the Magellanic Clouds

552 citations · 4.2k across the 59 of their papers we have counts for

collaborators
Showing 2016Show all

4 papers · 1 filter

astro-ph.GA2016★ 8 cited

Is there substructure around M87?

L. J. Oldham, N. W. Evans

We present a general method to identify infalling substructure in discrete datasets with position and line-of-sight velocity data. We exploit the fact that galaxies falling onto a…

astro-ph.GA2016

The Gaia-ESO survey: Metal-rich bananas in the bulge

Angus A. Williams, N. W. Evans, Matthew Molloy +25

We analyse the kinematics of ∼2000 giant stars in the direction of the Galactic bulge, extracted from the Gaia-ESO survey in the region $-10^\circ \lesssim \ell \lesssim 10^\…

astro-ph.GA2016

Is the Dark Halo of the Milky Way Prolate?

A. Bowden, N. W. Evans, A. A. Williams

We introduce the flattening equation, which relates the shape of the dark halo to the angular velocity dispersions and the density of a tracer population of stars. It assumes spher…

astro-ph.GA2016

Discy dwarf disruption and the shape of the Galactic halo

S. L. J. Gibbons, V. Belokurov, D. Erkal +1

The shape of the Galactic dark halo can, in principle, be inferred through modelling of stellar tidal streams in the Milky Way halo. The brightest and the longest of these, the Sag…

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