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researcher

A. Udalski

147 papers hereh-index 378 citations31 works total

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

author position
  • first author1
  • middle author96
  • last author6

Across the 103 of 147 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP63
  • astro-ph.SR54
  • astro-ph.GA20
  • astro-ph.HE6
  • astro-ph.IM2
  • astro-ph1
same name
  • A. Udalski — 577 papers, h 72
  • A. Udalski — 13 papers, h 26
  • A. Udalski — 7 papers
  • A. Udalski — 5 papers, 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

activity
20082026
most citedOne or more bound planets per Milky Way star from microlensing observations

588 citations · 5.8k across the 140 of their papers we have counts for

collaborators
Showing 2009Show all

3 papers · 1 filter

astro-ph.GA2009★ 88 cited

Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. II. Ages, metallicities, detailed elemental abundances, and connections to the Galactic thick disc

T. Bensby, S. Feltzing, J. A. Johnson +13

The Bulge is the least understood major stellar population of the Milky Way. Most of what we know about the formation and evolution of the Bulge comes from bright giant stars. The…

astro-ph.GA2009★ 160 cited

The Extreme Microlensing Event OGLE-2007-BLG-224: Terrestrial Parallax Observation of a Thick-Disk Brown Dwarf

A. Gould, A. Udalski, B. Monard +10

Parallax is the most fundamental technique to measure distances to astronomical objects. Although terrestrial parallax was pioneered over 2000 years ago by Hipparchus (ca. 140 BCE)…

astro-ph.GA2009★ 30 cited

Chemical evolution of the Galactic bulge as traced by microlensed dwarf and subgiant stars. Detailed abundance analysis of OGLE-2008-BLG-209S

T. Bensby, J. A. Johnson, J. Cohen +7

AIMS. Our aims are twofold. First we aim to evaluate the robustness and accuracy of stellar parameters and detailed elemental abundances that can be derived from high-resolution sp…

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