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P. G. Williams

45 papers hereh-index 305.3k citations70 works total

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

author position
  • first author3
  • middle author16
  • last author13

Across the 32 of 45 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE36
  • astro-ph.SR3
  • astro-ph.CO2
  • astro-ph.EP2
  • astro-ph.GA1
  • cs.DL1

identity via Semantic Scholar / OpenAlex

activity
20132026
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 6.8k across the 45 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

3 papers · 1 filter

astro-ph.SR2019★ 25 cited

Signs of accretion in the white dwarf + brown dwarf binary NLTT5306

E. S. Longstaff, S. L. Casewell, G. A. Wynn +4

We present new XSHOOTER spectra of NLTT5306, a 0.44 ± 0.04\msun white dwarf in a short period (101\,min) binary system with a brown dwarf companion that is likely to have previ…

astro-ph.SR2015★ 49 cited

The Rotation Period and Magnetic Field of the T Dwarf 2MASSI J1047539+212423 Measured From Periodic Radio Bursts

P. K. G. Williams, E. Berger

Periodic radio bursts from very low mass stars and brown dwarfs simultaneously probe their magnetic and rotational properties. The brown dwarf 2MASSI J1047539+212423 (2M 1047+21) i…

astro-ph.SR2013★ 103 cited

Trends in Ultracool Dwarf Magnetism. I. X-Ray Suppression and Radio Enhancement

P. K. G. Williams, B. A. Cook, E. Berger

Although ultracool dwarfs (UCDs) are now known to generate and dissipate strong magnetic fields, a clear understanding of the underlying dynamo is still lacking. We have performed…

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