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researcher

K. Pan

3 papers here

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

author position
  • middle author2

Across the 2 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE1
  • astro-ph.SR1
  • physics.ins-det1
ORCID 0000-0002-1473-9880
same name
  • K. Pan — 37 papers, h 80
  • K. Pan — 3 papers, h 10
  • K. Pan — 2 papers, h 11
  • K. Pan — 1 paper
  • K. Pan — 1 paper, h 15

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

most citedFeatures of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae

42 citations · 82 across the 3 of their papers we have counts for

collaborators

3 papers

physics.ins-det2019★ 16 cited

An arm length stabilization system for KAGRA and future gravitational-wave detectors

T. Akutsu, M. Ando, K. Arai +198

Modern ground-based gravitational wave (GW) detectors require a complex interferometer configuration with multiple coupled optical cavities. Since achieving the resonances of the a…

astro-ph.HE2019★ 42 cited

Features of Accretion-phase Gravitational-wave Emission from Two-dimensional Rotating Core-collapse Supernovae

Michael A. Pajkos, Sean M. Couch, Kuo-Chuan Pan +1

We explore the influence of progenitor mass and rotation on the gravitational-wave (GW) emission from core-collapse supernovae, during the postbounce, preexplosion, accretion-phase…

astro-ph.SR2017★ 24 cited

Physical Structures of the Type Ia Supernova Remnant N103B

Chuan-Jui Li, You-Hua Chu, Robert A. Gruendl +6

N103B is a Type Ia supernova remnant (SNR) projected in the outskirt of the superbubble around the rich cluster NGC 1850 in the Large Magellanic Cloud (LMC). We have obtained Hα…

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