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researcher

Shuai Zhang

3 papers here

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

fields
  • astro-ph.HE3
ORCID 0000-0003-2413-9587
same name
  • Shuai Zhang — 14 papers
  • Shuai Zhang — 13 papers, h 15
  • Shuai Zhang — 13 papers
  • Shuai Zhang — 8 papers, h 16
  • Shuai Zhang — 8 papers
  • Shuai Zhang — 7 papers, h 10

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

most citedEvaluating the bulk Lorentz factors of outflow material: lessons learned from the extremely-energetic outburst GRB 160625B

23 citations · 53 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2016★ 17 cited

The interpretation of the multi-wavelength afterglow emission of short GRB 140903A

Shuai Zhang, Zhi-Ping Jin, Yuan-Zhu Wang +1

GRB 140903A, a short duration γ−ray burst (SGRB) detected by {\it Swift}, is characterized by its long-lasting radio emission among SGRBs. In addition to the ∼106 s radi…

astro-ph.HE2016★ 23 cited

Evaluating the bulk Lorentz factors of outflow material: lessons learned from the extremely-energetic outburst GRB 160625B

Yuan-Zhu Wang, Hao Wang, Shuai Zhang +6

GRB 160625B is an extremely-bright outburst with well-monitored afterglow emission. The geometry-corrected energy is high up to ∼5.2×1052 erg or even $\sim 8\times 10…

astro-ph.HE2014★ 13 cited

The magnetization degree of the outflow powering the highly-polarized reverse shock emission of GRB 120308A

Shuai Zhang, Zhi-Ping Jin, Da-Ming Wei

GRB 120308A, a long duration γ−ray burst detected by {\it Swift}, was distinguished by a highly-polarized early optical afterglow emission that strongly suggests an ordered magne…

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