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researcher

L. Williams

111 papers hereh-index 302.7k citations142 works total

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

author position
  • sole author2
  • first author22
  • middle author44
  • last author35

Across the 103 of 111 papers where every author was matched, so the position is known.

fields
  • astro-ph.CO47
  • astro-ph40
  • astro-ph.GA24
same name
  • L. Williams — 61 papers, h 34
  • L. Williams — 19 papers
  • L. Williams — 17 papers, h 70
  • L. Williams — 11 papers, h 5
  • L. Williams — 10 papers, h 43
  • L. Williams — 7 papers, h 9

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
19952025
most citedThe Frontier Fields Lens Modeling Comparison Project

233 citations · 3.3k across the 110 of their papers we have counts for

collaborators
Showing 2003Show all

4 papers · 1 filter

astro-ph2003★ 106 cited

Investigating the Origins of Dark Matter Halo Density Profiles

Liliya L. R. Williams, Arif Babul, Julianne J. Dalcanton

Although high-resolution N-body simulations make robust empirical predictions for the density distribution within cold dark matter halos, these studies have yielded little physical…

astro-ph2003★ 19 cited

Is B1422+231 a Golden Lens?

Somak Raychaudhury, Prasenjit Saha, Liliya L. R. Williams

B1422+231 is a quadruply-imaged QSO with an exceptionally large lensing contribution from group galaxies other than the main lensing galaxy. We detect diffuse X-rays from the galax…

astro-ph2003★ 65 cited

Qualitative Theory for Lensed QSOs

Prasenjit Saha, Liliya L. R. Williams

We show that some characteristics of multiply-imaged QSO systems are very model-independent and can be deduced accurately by simply scrutinizing the relative positions of images an…

astro-ph2003★ 12 cited

Determination of Reddening and Extinction Due to Dust in APM Galaxy Clusters

Joshua G. Nollenberg, Liliya L. R. Williams, Steve J. Maddox

Existing observations are consistent with rich clusters of galaxies having no dust on $\simgt$ Mpc scales, while galaxy groups most probably do have dust distributed over $\lesssim…

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