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researcher

K. Maeda

166 papers hereh-index 6517.5k citations546 works total

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

author position
  • sole author3
  • first author20
  • middle author80
  • last author57

Across the 160 of 166 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE64
  • astro-ph33
  • gr-qc28
  • hep-th25
  • astro-ph.SR11
  • astro-ph.GA2
same name
  • K. Maeda — 68 papers, h 31
  • K. Maeda — 19 papers, h 5
  • K. Maeda — 15 papers, h 8
  • K. Maeda — 12 papers, h 14
  • K. Maeda — 12 papers, h 4
  • K. Maeda — 9 papers, h 16

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
19952023
most citedMeasurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow

457 citations · 3.6k across the 77 of their papers we have counts for

collaborators
Showing 2015 · astro-ph.HEShow all

3 papers · 2 filters

astro-ph.HE2015★ 84 cited

A systematic study of carbon-oxygen white dwarf mergers: mass combinations for Type Ia supernovae

Yushi Sato, Naohito Nakasato, Ataru Tanikawa +3

Mergers of two carbon-oxygen (CO) white dwarfs (WDs) have been considered as progenitors of Type Ia supernovae (SNe Ia). Based on smoothed particle hydrodynamics (SPH) simulations,…

astro-ph.HE2015★ 2 cited

Hydrodynamical evolution of merging carbon-oxygen white dwarfs: their pre-supernova structure and observational counterparts

Ataru Tanikawa, Naohito Nakasato, Yushi Sato +3

We perform smoothed particle hydrodynamics (SPH) simulations for merging binary carbon-oxygen (CO) white dwarfs (WDs) with masses of 1.1 and 1.0 M⊙​, until the merger rem…

astro-ph.HE2015★ 131 cited

A Chandrasekhar Mass Progenitor for the Type Ia Supernova Remnant 3C 397 from The Enhanced Abundances of Nickel and Manganese

Hiroya Yamaguchi, Carles Badenes, Adam R. Foster +8

Despite decades of intense efforts, many fundamental aspects of Type Ia supernova (SNe Ia) remain elusive. One of the major open questions is whether the mass of the exploding whit…

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