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K. Toma

9 papers hereh-index 4214.9k citations144 works total

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

author position
  • first author2
  • middle author6
  • last author1

Across the 9 of 9 papers where every author was matched, so the position is known.

fields
  • astro-ph5
  • astro-ph.HE4
same name
  • K. Toma — 1 paper, h 5

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
20042011
most citedDiscerning the physical origins of cosmological Gamma-ray bursts based on multiple observational criteria: the cases of z=6.7 GRB 080913, z=8.3 GRB 090423, and some short/hard GRBs

440 citations · 521 across the 6 of their papers we have counts for

collaborators
Showing 2005Show all

3 papers · 1 filter

astro-ph2005

Efficiency Crisis of Swift Gamma-Ray Bursts with Shallow X-ray Afterglows: Prior Activity or Time-Dependent Microphysics?

Kunihito Ioka, Kenji Toma, Ryo Yamazaki +1

Most X-ray afterglows of gamma-ray bursts (GRBs) observed by the Swift satellite have a shallow decay phase t^{-1/2} in the first few hours. This is not predicted by the standard a…

astro-ph2005

Shallow Decay of Early X-ray Afterglows from Inhomogeneous Gamma-Ray Burst Jets

Kenji Toma, Kunihito Ioka, Ryo Yamazaki +1

Almost all the X-ray afterglows of gamma-ray bursts (GRBs) observed by the Swift satellite have a shallow decay phase in the first thousands of seconds. We show that in an inhomoge…

astro-ph2005

A Unified Model for Gamma-Ray Bursts

Ryo Yamazaki, Kunihito Ioka, Takashi Nakamura +1

A possible unified model of short and long gamma-ray bursts (GRBs), X-ray rich GRBs, and X-ray flashes is proposed. It is assumed that the jet of a GRB consists of many emitting su…

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