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T. Sakamoto

4 papers hereh-index 23.1k citations5 works total

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

author position
  • middle author3
  • last author1

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • T. Sakamoto — 68 papers, h 52
  • T. Sakamoto — 17 papers, h 16
  • T. Sakamoto — 16 papers, h 22
  • T. Sakamoto — 10 papers, h 8
  • T. Sakamoto — 8 papers, h 27
  • T. Sakamoto — 6 papers

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
20162024
collaborators

4 papers

astro-ph.HE2024

Characterization of a peculiar Einstein Probe transient EP240408a: an exotic gamma-ray burst or an abnormal jetted tidal disruption event?

B. O'Connor, D. Pasham, I. Andreoni +30

We present the results of our multi-wavelength (X-ray to radio) follow-up campaign of the Einstein Probe transient EP240408a. The initial 10 s trigger displayed bright soft X-ray (…

astro-ph.HE2024

Searching for the Signature of Fast Radio Burst by Swift/XRT X-ray Afterglow Light Curve

Hsien-chieh Shen, Takanori Sakamoto, Motoko Serino +1

A new type of cosmological transient, dubbed fast radio bursts (FRBs), was recently discovered. The source of FRBs is still unknown. One possible scenario of an FRB is the collapse…

astro-ph.HE2018

The outflow structure of GW170817 from late time broadband observations

E. Troja, L. Piro, G. Ryan +6

We present our broadband study of GW170817 from radio to hard X-rays, including NuSTAR and Chandra observations up to 165 days after the merger, and a multi-messenger analysis incl…

astro-ph.HE2016

An achromatic break in the afterglow of the short GRB 140903A: evidence for a narrow jet

E. Troja, T. Sakamoto, S. B. Cenko +17

We report the results of our observing campaign on GRB140903A, a nearby (z=0.351) short duration (T90~0.3 s) gamma-ray burst discovered by Swift. We monitored the X-ray afterglow w…

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