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researcher

K. Kashiyama

79 papers hereh-index 262k citations92 works total

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

author position
  • first author17
  • middle author48
  • last author12

Across the 77 of 79 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE61
  • astro-ph.GA6
  • astro-ph.SR6
  • astro-ph.CO4
  • astro-ph.IM1
  • gr-qc1
same name
  • K. Kashiyama — 1 paper, h 13
  • K. Kashiyama — 1 paper, h 7

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
20092026
most citedA Burst in a Wind Bubble and the Impact on Baryonic Ejecta: High-Energy Gamma-Ray Flashes and Afterglows from Fast Radio Bursts and Pulsar-Driven Supernova Remnants

256 citations · 2.5k across the 78 of their papers we have counts for

collaborators
Showing 2019Show all

3 papers · 1 filter

astro-ph.HE2019★ 39 cited

A Search for Late-Time Radio Emission and Fast Radio Bursts from Superluminous Supernovae

C. J. Law, C. M. B. Omand, K. Kashiyama +10

We present results of a search for late-time radio emission and Fast Radio Bursts (FRBs) from a sample of type-I superluminous supernovae (SLSNe-I). We used the Karl G. Jansky Very…

astro-ph.SR2019★ 19 cited

The optically thick rotating magnetic wind from a massive white dwarf merger product

Kazumi Kashiyama, Kotaro Fujisawa, Toshikazu Shigeyama

WD J005311 is a newly identified white dwarf (WD) in a mid-infrared nebula. The spectroscopic observation indicates the existence of a neon-enriched carbon/oxygen wind with a termi…

astro-ph.HE2019★ 25 cited

Type IIn Supernova Light Curves Powered by Forward and Reverse Shocks

Daichi Tsuna, Kazumi Kashiyama, Toshikazu Shigeyama

We present a bolometric light curve model of Type IIn supernovae powered by supernova ejecta colliding with a circumstellar medium. We estimate the conversion efficiency of the eje…

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