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researcher

A. McWilliam

64 papers hereh-index 447.2k citations208 works total

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

author position
  • sole author3
  • first author6
  • middle author31
  • last author20

Across the 60 of 64 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA25
  • astro-ph22
  • astro-ph.SR14
  • astro-ph.CO2
  • astro-ph.HE1
same name
  • A. McWilliam — 9 papers, h 7
  • A. McWilliam — 6 papers, h 7
  • A. McWilliam — 6 papers, h 5

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
19992023
most citedThe Galactic Thick Disk Stellar Abundances

422 citations · 4.4k across the 64 of their papers we have counts for

collaborators
Showing 2010 · astro-ph.GAShow all

4 papers · 2 filters

astro-ph.GA2010★ 1 cited

Galactic chemical evolution: the observational side

Andrew McWilliam

In this review I outline some ideas in chemical evolution, necessary for understanding the evolution of galaxies from measured elemental abundance ratios. I then discuss abundance…

astro-ph.GA2010★ 306 cited

Two Red Clumps and the X-Shaped Milky Way Bulge

Andrew McWilliam, Manuela Zoccali

From 2MASS infra-red photometry we find two red clump (RC) populations co-existing in the same fields toward the Galactic bulge at latitudes |b|>5.5 deg., ranging over ~13 degrees…

astro-ph.GA2010★ 23 cited

A differential chemical abundance scale for the globular cluster M5

Andreas Koch, Andrew McWilliam

We present LTE chemical abundances for five red giants and one AGB star in the Galactic globular cluster (GC) M5 based on high resolution spectroscopy using the MIKE spectrograph o…

astro-ph.GA2010★ 133 cited

High-Resolution Spectroscopy of Extremely Metal-Poor Stars in the Least Evolved Galaxies: Leo IV

Joshua D. Simon, Anna Frebel, Andrew McWilliam +2

We present high-resolution Magellan/MIKE spectroscopy of the brightest star in the ultra-faint dwarf galaxy Leo IV. We measure an iron abundance of [Fe/H] = -3.2, adding to the rap…

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