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researcher

M. Collins

51 papers hereh-index 242.6k citations66 works total

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

author position
  • first author12
  • middle author35
  • last author1

Across the 48 of 51 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA39
  • astro-ph.CO9
  • astro-ph1
  • astro-ph.IM1
  • astro-ph.SR1
same name
  • M. Collins — 14 papers, h 13
  • M. Collins — 11 papers, h 24
  • M. Collins — 9 papers, h 5
  • M. Collins — 8 papers, h 48
  • M. Collins — 5 papers, h 3
  • M. Collins — 4 papers, h 3

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
20082023
most citedThe remnants of galaxy formation from a panoramic survey of the region around M31

623 citations · 3k across the 51 of their papers we have counts for

collaborators
Showing 2013Show all

3 papers · 1 filter

astro-ph.GA2013★ 276 cited

The large-scale structure of the halo of the Andromeda Galaxy Part I: global stellar density, morphology and metallicity properties

Rodrigo A. Ibata, Geraint F. Lewis, Alan W. McConnachie +14

We present an analysis of the large-scale structure of the halo of the Andromeda galaxy, based on the Pan-Andromeda Archeological Survey (PAndAS), currently the most complete map o…

astro-ph.CO2013★ 77 cited

The masses of Local Group dwarf spheroidal galaxies: The death of the universal mass profile

Michelle L. M. Collins, Scott C. Chapman, R. M. Rich +12

We investigate the claim that all dwarf spheroidal galaxies (dSphs) reside within halos that share a common, universal mass profile as has been derived for dSphs of the Galaxy. By…

astro-ph.CO2013★ 184 cited

A kinematic study of the Andromeda dwarf spheroidal system

Michelle L. M. Collins, Scott C. Chapman, R. Michael Rich +12

We present a homogeneous kinematic analysis of red giant branch stars within 18 of the 28 Andromeda dwarf spheroidal (dSph) galaxies, obtained using the Keck I LRIS and Keck II DEI…

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