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researcher

W. Wilson

22 papers hereh-index 182.5k citations62 works total

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

author position
  • middle author9
  • last author10

Across the 19 of 22 papers where every author was matched, so the position is known.

fields
  • astro-ph11
  • astro-ph.CO6
  • astro-ph.IM4
  • astro-ph.GA1
same name
  • W. Wilson — 13 papers, h 16
  • W. Wilson — 7 papers, h 4
  • W. Wilson — 4 papers, h 27
  • W. Wilson — 4 papers, h 12
  • W. Wilson — 2 papers, h 3
  • W. Wilson — 1 paper, h 64

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
19962012
most citedThe Parkes Pulsar Timing Array Project

509 citations · 2k across the 22 of their papers we have counts for

collaborators
Showing 2008Show all

4 papers · 1 filter

astro-ph2008★ 14 cited

Tests of AMiBA Data Integrity

Hiroaki Nishioka, Fu-Cheng Wang, Jiun-Huei Proty Wu +26

We describe methods used to validate data from the Y.T. Lee Array for Microwave Background Anisotropy (AMiBA), an interferometric array designed to measure the Sunyaev-Zel'dovich e…

astro-ph2008★ 38 cited

The Yuan-Tseh Lee Array for Microwave Background Anisotropy

Paul T. P. Ho, Pablo Altamirano, Chia-Hao Chang +52

The Yuan-Tseh Lee Array for Microwave Background Anisotropy (AMiBA) is the first interferometer dedicated to studying the cosmic microwave background (CMB) radiation at 3mm wavelen…

astro-ph2008★ 115 cited

Mass and Hot Baryons in Massive Galaxy Clusters from Subaru Weak Lensing and AMiBA SZE Observations

Keiichi Umetsu, Mark Birkinshaw, Guo-Chin Liu +30

We present a multiwavelength analysis of a sample of four hot (T_X>8keV) X-ray galaxy clusters (A1689, A2261, A2142, and A2390) using joint AMiBA Sunyaev-Zel'dovich effect (SZE) an…

astro-ph2008★ 18 cited

The Coherent Radio Emission from the RS CVn Binary HR 1099

O. B. Slee, W. Wilson, G. Ramsay

We used the Australia Telescope in March-April 2005 to observe the RS CVn binary HR 1099 at 1.384 and 2.368 GHz at two epochs, each of 9 h in duration and 11 days apart. During two…

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