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D. M. Alexander

3 papers hereh-index 127 citations3 works total

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

author position
  • first author1
  • middle author1

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3
same name
  • D. M. Alexander — 23 papers, h 6
  • D. M. Alexander — 11 papers, h 5
  • D. M. Alexander — 9 papers, h 6
  • D. M. Alexander — 4 papers
  • D. M. Alexander — 1 paper, 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

most citedAn enhanced merger fraction within the galaxy population of the SSA22 protocluster at z ~ 3.1

57 citations · 130 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2016★ 50 cited

Herschel protocluster survey: A search for dusty star-forming galaxies in protoclusters at z=2-3

Y. Kato, Y. Matsuda, Ian Smail +15

We present a Herschel/SPIRE survey of three protoclusters at z=2-3 (2QZCluster, HS1700, SSA22). Based on the SPIRE colours (S350/S250 and S500/S350) of 250 μm sources, we selecte…

astro-ph.GA2016★ 23 cited

ALMA observations of a z~3.1 Protocluster: Star Formation from Active Galactic Nuclei and Lyman-Alpha Blobs in an Overdense Environment

D. M. Alexander, J. M. Simpson, C. M. Harrison +14

We exploit ALMA 870um observations to measure the star-formation rates (SFRs) of eight X-ray detected Active Galactic Nuclei (AGNs) in a z~3.1 protocluster, four of which reside in…

astro-ph.GA2015★ 57 cited

An enhanced merger fraction within the galaxy population of the SSA22 protocluster at z ~ 3.1

N. K. Hine, J. E. Geach, D. M. Alexander +3

The over-dense environments of protoclusters of galaxies in the early Universe (z>2) are expected to accelerate the evolution of galaxies, with an increased rate of stellar mass as…

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