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researcher

K. Maeda

69 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 author14
  • middle author27
  • last author22

Across the 66 of 69 papers where every author was matched, so the position is known.

fields
  • astro-ph33
  • hep-th21
  • gr-qc10
  • astro-ph.HE3
  • astro-ph.CO1
  • astro-ph.GA1
same name
  • K. Maeda — 8 papers, h 31
  • K. Maeda — 7 papers, h 8
  • K. Maeda — 5 papers, h 16
  • K. Maeda — 5 papers, h 20
  • K. Maeda — 3 papers, h 12
  • K. Maeda — 2 papers, h 3

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
19952012
most citedMeasurement of the Kerr Spin Parameter by Observation of a Compact Object's Shadow

457 citations · 2.3k across the 37 of their papers we have counts for

collaborators
Showing 2003 · astro-phShow all

3 papers · 2 filters

astro-ph2003

Dust in the Early Universe: Dust Formation in the Ejecta of Population III Supernovae

Takaya Nozawa, Takashi Kozasa, Hideyuki Umeda +2

We investigate the formation of dust grains in the ejecta of population III supernovae including pair--instability supernovae, applying a theory of non-- steady state nucleation an…

astro-ph2003

Nucleosynthesis in Black-Hole-Forming Supernovae and Abundance Patterns of Extremely Metal-Poor Stars

K. Nomoto, K. Maeda, H. Umeda +4

Stars more massive than ∼ 20 - 25 \ms form a black hole at the end of their evolution. Stars with non-rotating black holes are likely to collapse "quietly" ejecting a small am…

astro-ph2003

A Two-Component Model for the Light Curves of Hypernovae

K. Maeda, P. A. Mazzali, J. Deng +4

The light curves of 'hypernovae', i.e. very energetic supernovae with E51​≡E/1051ergs $\gsim 5-10$ are characterized at epochs of a few months by a phase of linear de…

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