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GeV Emission during X-Ray Flares from Late Internal Shocks: Application to GRB 100728A

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Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
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K. Wang, Z. G. Dai (NJU)

High Energy Astrophysical Phenomena · Submitted 6 Aug 2013

abstract compiled · 2026-09-23 · no language-model review

The authors' main claim By analytical and numerical calculations, the observed spectral properties in GRB 100728A can be well explained.

how it is stated · asserted 0.96 read the record →

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arXiv ID1308.1248 (version 1)
Pith ID3N75ICHY, Pith's permanent record of this paper and its review
CitationK. Wang, Z. G. Dai (NJU). "GeV Emission during X-Ray Flares from Late Internal Shocks: Application to GRB 100728A." arXiv:1308.1248 (2013). https://pith.science/paper/3N75ICHY
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The compiled record

The paper's own sentences, arranged. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.

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Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 3,622 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.05 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.07 · compares with prior results 0.13 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v1. Results and the main claim are underlined; .

Recently, the GeV radiation during the X-ray flare activity in GRB 100728A was detected by Feimi/LAT. Here we study the dynamics and emission properties of collision between two homogeneous shells based on the late internal shock model. The GeV photons can be produced from X-ray flare photons up-scattered by relativistic electrons accelerated by forward-reverse shocks, where involved radiative processes include synchrotron self-Compton and crossing inverse-Compton scattering. By analytical and numerical calculations, the observed spectral properties in GRB 100728A can be well explained.

background contribution method result interpretation main claim

What the classifier reports for each sentence. The number is the probability it gave the label.
#sentencerolethe authors' own workstates the main conclusionstrength
s0 Recently, the GeV radiation during the X-ray flare activity in GRB 100728A was detected by Feimi/LAT. background 0.99 0.08 0.04 asserted 1.00
s1 Here we study the dynamics and emission properties of collision between two homogeneous shells based on the late internal shock model. contribution 0.87 0.86 0.04 asserted 0.88
s2 The GeV photons can be produced from X-ray flare photons up-scattered by relativistic electrons accelerated by forward-reverse shocks, where involved radiative processes include synchrotron self-Compton and crossing inverse-Compton scattering. method 0.74 0.45 0.20 asserted 0.78
s3 By analytical and numerical calculations, the observed spectral properties in GRB 100728A can be well explained. result 0.97 0.91 0.77 asserted 0.96

What kind of paper the classifier reports this is: theoretical result 0.95 · evidence from simulation or computation 0.77.

What was examined, and what was not

sources read
  • arXiv listing abstract v1
not examined
  • full text
  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
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  • S sections
  • T body sentences
  • C citations
  • R cross-paper relations

Every quoted sentence on this record is the authors'. Every label is from Pith's closed vocabulary, with the probability shown beside it. Every number in the measurements table is the authors', checked by code. Record as JSON

The paper
Original abstract

Recently, the GeV radiation during the X-ray flare activity in GRB 100728A was detected by Feimi/LAT. Here we study the dynamics and emission properties of collision between two homogeneous shells based on the late internal shock model. The GeV photons can be produced from X-ray flare photons up-scattered by relativistic electrons accelerated by forward-reverse shocks, where involved radiative processes include synchrotron self-Compton and crossing inverse-Compton scattering. By analytical and numerical calculations, the observed spectral properties in GRB 100728A can be well explained.

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