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M. Taylor

24 papers hereh-index 14583 citations31 works total

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

author position
  • first author6
  • middle author14
  • last author2

Across the 22 of 24 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA20
  • astro-ph.IM2
  • astro-ph.CO1
  • astro-ph.EP1
same name
  • M. Taylor — 13 papers, h 5
  • M. Taylor — 10 papers, h 7
  • M. Taylor — 10 papers, h 7
  • M. Taylor — 9 papers, h 2
  • M. Taylor — 7 papers, h 40
  • M. Taylor — 6 papers, h 15

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
20102026
most citedThe Canada-France Ecliptic Plane Survey - Full Data Release: The orbital structure of the Kuiper belt

287 citations · 1.2k across the 23 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.GA2019★ 12 cited

The Next Generation Fornax Survey (NGFS): VI. The Alignment of Dwarf Galaxies in The Fornax Cluster

Yu Rong, Thomas H. Puzia, Paul Eigenthaler +16

Using the photometric data from the Next Generation Fornax Survey, we find a significant radial alignment signal among the Fornax dwarf galaxies. For the first time, we report that…

astro-ph.IM2019★ 37 cited

The Detailed Science Case for the Maunakea Spectroscopic Explorer, 2019 edition

The MSE Science Team, Carine Babusiaux, Maria Bergemann +258

(Abridged) The Maunakea Spectroscopic Explorer (MSE) is an end-to-end science platform for the design, execution and scientific exploitation of spectroscopic surveys. It will unvei…

astro-ph.GA2019★ 7 cited

The Next Generation Fornax Survey (NGFS): V. Discovery of a dwarf-dwarf galaxy pair at z=0.30 and its characterization using deep VLT/MUSE observations

Evelyn J. Johnston, Paul Eigenthaler, Thomas Puzia +11

We report the detection of a pair of dwarf galaxies at z=0.30 which may be in the early stages of an interaction. Both galaxies have stellar masses of <109M⊙​, and d…

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