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D. Tak

4 papers hereh-index 8258 citations25 works total

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

author position
  • first author1
  • middle author2

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

fields
  • astro-ph.HE4
same name
  • D. Tak — 7 papers, h 14
  • D. Tak — 6 papers, h 9
  • D. Tak — 1 paper, h 1
  • D. Tak — 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

collaborators

4 papers

astro-ph.HE2026

Evidence of High-latitude Emission in the Prompt Phase of GRBs: How Far from the Central Engine are the GRBs Produced?

Z. Lucas Uhm, Donggeun Tak, Bing Zhang +5

One of the difficulties in nailing down the physical mechanism of gamma-ray bursts (GRBs) comes from the fact that there has been no clear observational evidence on how far from th…

astro-ph.HE2025

Deciphering the Physical Origin of GRB 240825A: A Long GRB Lacking a Bright Supernova

Rahul Gupta, Judith L. Racusin, R. Sanchez-Ramirez +52

We present a comprehensive multiwavelength analysis of GRB 240825A, a bright gamma-ray burst (GRB) detected by Fermi and Swift, with a prompt duration (T90​ ~ 4 sec in 50-3…

astro-ph.HE2025

An in-depth study of Gamma rays from the Starburst Galaxy M 82 with VERITAS

Atreya Acharyya, Colin B. Adams, Priyadarshini Bangale +60

Assuming Galactic cosmic rays originate in supernovae and the winds of massive stars, starburst galaxies should produce very-high-energy (VHE; E>100 GeV) gamma-ray emission via t…

astro-ph.HE2025

Multiwavelength Afterglow Analysis of GRB 221009A: Unveiling the Evolution of a Cooling Break in a Wind-like Medium

Donggeun Tak, Z. Lucas Uhm, Gregory S. H. Paek +8

Gamma-ray bursts (GRBs) are the most energetic explosions in the universe, and their afterglow emission provides an opportunity to probe the physics of relativistic shock waves in…

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