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Y. Chu

47 papers hereh-index 275.4k citations76 works total

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

author position
  • first author2
  • middle author8

Across the 10 of 47 papers where every author was matched, so the position is known.

fields
  • gr-qc20
  • astro-ph.HE14
  • astro-ph.IM7
  • astro-ph.CO3
  • physics.ins-det2
  • hep-ph1
same name
  • Y. Chu — 158 papers, h 43
  • Y. Chu — 111 papers, h 32
  • Y. Chu — 29 papers, h 12
  • Y. Chu — 27 papers, h 78
  • Y. Chu — 22 papers, h 23
  • Y. Chu — 21 papers, h 18

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
20142026
most citedGWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run

1.8k citations · 4.7k across the 45 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.HE2020★ 51 cited

Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1589

We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and…

gr-qc2020★ 9 cited

Overview of KAGRA : KAGRA science

KAGRA Collaboration, T. Akutsu, M. Ando +240

KAGRA is a newly build gravitational-wave observatory, a laser interferometer with 3 km arm length, located in Kamioka, Gifu, Japan. In this paper in the series of KAGRA-featured a…

gr-qc2020★ 9 cited

Spherical harmonic analysis of anisotropies in polarized stochastic gravitational wave background with interferometry experiments

Yu-Kuang Chu, Guo-Chin Liu, Kin-Wang Ng

We study the interferometric observation of intensity and polarization anisotropies of a stochastic gravitational wave background (SGWB). We show that the observed correlated data…

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