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researcher

H. Yamamoto

54 papers here

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

author position
  • last author1

Across the 1 of 54 papers where every author was matched, so the position is known.

fields
  • gr-qc23
  • astro-ph.HE16
  • hep-ex9
  • astro-ph.CO2
  • astro-ph.IM2
  • astro-ph1
ORCID 0000-0001-6919-9570
same name
  • H. Yamamoto — 144 papers, h 82
  • H. Yamamoto — 66 papers, h 28
  • H. Yamamoto — 63 papers, h 29
  • H. Yamamoto — 51 papers
  • H. Yamamoto — 27 papers, h 25
  • H. Yamamoto — 24 papers, h 12

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
19972026
most citedGravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

3.6k citations · 10.5k across the 54 of their papers we have counts for

collaborators
Showing 2024Show all

3 papers · 1 filter

astro-ph.HE2024★ 14 cited

Search for gravitational waves emitted from SN 2023ixf

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1780

We present the results of a search for gravitational-wave transients associated with core-collapse supernova SN 2023ixf, which was observed in the galaxy Messier 101 via optical em…

astro-ph.HE2024★ 5 cited

A search using GEO600 for gravitational waves coincident with fast radio bursts from SGR 1935+2154

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1780

The magnetar SGR 1935+2154 is the only known Galactic source of fast radio bursts (FRBs). FRBs from SGR 1935+2154 were first detected by CHIME/FRB and STARE2 in 2020 April, after t…

astro-ph.HE2024★ 201 cited

Observation of Gravitational Waves from the Coalescence of a 2.5-4.5 M⊙​ Compact Object and a Neutron Star

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1793

We report the observation of a coalescing compact binary with component masses 2.5-4.5 M⊙​ and 1.2-2.0 M⊙​ (all measurements quoted at the 90% credible le…

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