Pith. Sign in

RECORD

Detection of High-Energy Gamma-Ray Emission during the X-ray flaring activity in GRB100728A

PaperPDF from arXiv

data files

Paper breakdownThe authors' claims, conditions and measurements, as JSON Signed receiptProof this review has not been altered
X Bluesky LinkedIn Reddit Hacker News
The Fermi Collaboration, L. Piro

High Energy Astrophysical Phenomena · Submitted 28 Apr 2011

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

The authors' main claim In the same time interval high energy emission is significantly detected by the Fermi/LAT.

how it is stated · asserted 1.00 read the record →

Comment (0) Read on arXiv ↗
Cite ▾
arXiv ID1104.5496 (version 1)
Pith IDS7SVXOTE, Pith's permanent record of this paper and its review
CitationL. Piro, The Fermi Collaboration. "Detection of High-Energy Gamma-Ray Emission during the X-ray flaring activity in GRB100728A." arXiv:1104.5496 (2011). https://pith.science/paper/S7SVXOTE
Claim paper

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.

Open the compiled record

Compiled by classifier-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,203 input tokens, $0.0002 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.35 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.50 · compares with prior results 0.08 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We present the simultaneous Swift and Fermi observations of the bright GRB100728A and its afterglow. The early X-ray emission is dominated by a vigorous flaring activity continuing until 1 ks after the burst. In the same time interval high energy emission is significantly detected by the Fermi/LAT. Marginal evidence of GeV emission is observed up to later times. We discuss the broadband properties of this burst within both the internal and external shock scenarios, with a particular emphasis on the relation between X-ray flares, the GeV emission and a continued long-duration central engine activity as their power source.

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 We present the simultaneous Swift and Fermi observations of the bright GRB100728A and its afterglow. contribution 0.90 0.94 0.04 asserted 0.99
s1 The early X-ray emission is dominated by a vigorous flaring activity continuing until 1 ks after the burst. result 1.00 0.81 0.07 asserted 1.00
s2 In the same time interval high energy emission is significantly detected by the Fermi/LAT. result 1.00 0.91 0.37 asserted 1.00
s3 Marginal evidence of GeV emission is observed up to later times. result 1.00 0.90 0.11 hedged possibility 0.85
s4 We discuss the broadband properties of this burst within both the internal and external shock scenarios, with a particular emphasis on the relation between X-ray flares, the GeV emission and a continued long-duration central engine activity as their power source. interpretation 0.54 0.58 0.21 unclear 0.67

What kind of paper the classifier reports this is: empirical study 1.00 · evidence from observation or experiment 0.85.

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
levels run
  • P abstract
not run
  • 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

We present the simultaneous Swift and Fermi observations of the bright GRB100728A and its afterglow. The early X-ray emission is dominated by a vigorous flaring activity continuing until 1 ks after the burst. In the same time interval high energy emission is significantly detected by the Fermi/LAT. Marginal evidence of GeV emission is observed up to later times. We discuss the broadband properties of this burst within both the internal and external shock scenarios, with a particular emphasis on the relation between X-ray flares, the GeV emission and a continued long-duration central engine activity as their power source.

Human review

How Pith checks papers → · Full audit of this paper →

References

Discussion

Know something about this paper? Leave a comment, or highlight any passage above to comment on it.