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researcher

Y. Sato

4 papers hereh-index 7175 citations30 works total

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

author position
  • first author2
  • middle author1

Across the 3 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4
same name
  • Y. Sato — 12 papers, h 16
  • Y. Sato — 10 papers, h 5
  • Y. Sato — 6 papers, h 2
  • Y. Sato — 5 papers, h 3
  • Y. Sato — 3 papers, h 2
  • Y. Sato — 3 papers, h 28

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

collaborators

4 papers

astro-ph.HE2026

Constraints on the VHE counterpart of two binary black hole mergers observed by the MAGIC and CTAO LST-1 telescopes

K. Abe, S. Abe, J. Abhir +439

We present very-high-energy gamma-ray observations of two binary black hole merger candidates, GW240615_113620 and GW241125_010116, performed with the Major Atmospheric Gamma Imagi…

astro-ph.HE2025

Interpreting the diversity of afterglow emission from radio-detected tidal disruption events with instantaneous and delayed outflows

Yuri Sato, Mukul Bhattacharya, Jose Carpio +2

Tidal disruption events (TDEs) occur when a star is gravitationally disrupted by the tidal field of a supermassive black hole during a close encounter. Radio emission has recently…

astro-ph.HE2025

Two-component jet model for the afterglow emission of GRB 201216C and GRB 221009A and implications for jet structure of very-high-energy gamma-ray bursts

Yuri Sato, Kohta Murase, Yutaka Ohira +2

In recent years, afterglow emission in the very-high-energy (VHE) band above 100 GeV has been clearly detected for at least five gamma-ray bursts (GRBs 180720B, 190114C, 190829A, 2…

astro-ph.HE2025

EP240414a: A Gamma-Ray Burst Jet Weakened by an Extended Circumstellar Material

Hamid Hamidani, Yuri Sato, Kazumi Kashiyama +3

The recent Einstein Probe (EP) event EP240414a exhibits several unusual observational features. Its prompt and afterglow emissions place it between long gamma-ray bursts (LGRBs) an…

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