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researcher

D. Williams

4 papers hereh-index 318 citations13 works total

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

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE2
  • astro-ph.CO1
  • astro-ph.IM1
same name
  • D. Williams — 39 papers, h 29
  • D. Williams — 13 papers, h 19
  • D. Williams — 3 papers, h 2
  • D. Williams — 3 papers, h 4
  • D. Williams — 2 papers
  • D. Williams — 1 paper, h 2

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
20242026
collaborators

4 papers

astro-ph.HE2026

IceCube Real-time Searches for High-energy Neutrinos Coincident with LIGO/Virgo/KAGRA Gravitational-Wave Alerts in O4a

The IceCube Collaboration, R. Abbasi, M. Ackermann +418

Gravitational-wave events from mergers of compact objects are a predicted source of high-energy neutrinos. Using data from the IceCube Neutrino Observatory, we search for neutrinos…

astro-ph.CO2026

The free-streaming length of dark matter from JWST observations of 28 strong gravitational lenses

D. Gilman, A. M. Nierenberg, T. Treu +24

The formation of gravitationally bound overdensities of dark matter (DM), or \textit{halos}, is a generic prediction of theories with particle DM. We present a measurement of halo…

astro-ph.IM2025

Narrowing RIFT: Focused simulation-based-inference for interpreting exceptional GW sources

Katelyn J. Wagner, R. O'Shaughnessy, A. Yelikar +6

The Rapid Iterative FiTting (RIFT) parameter inference algorithm provides a simulation-based inference approach to efficient, highly-parallelized parameter inference for GW sources…

astro-ph.HE2024

Efficient reanalysis of events from GWTC-3 with RIFT and asimov

D. Fernando, R. O'Shaughnessy, D. Williams

Different waveform models can yield notably different conclusions about the properties of individual gravitational wave events. For instance, previous analyses using the SEOBNRv4PH…

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