Pith. Sign in

RECORD

Gamma Ray Burst Prompt correlations

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
Maria Dainotti, Roberta Del Vecchio, Mariusz Tarnopolski

High Energy Astrophysical Phenomena · Submitted 2 Dec 2016

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

The authors' main claim However, GRBs spanning several orders of magnitude in their energetics are far from being standard candles.

how it is stated · asserted 1.00 read the record →

Comment (0) Read on arXiv ↗
Cite ▾
arXiv ID1612.00618 (version 4)
Pith IDDV5NO5AX, Pith's permanent record of this paper and its review
CitationMaria Dainotti, Mariusz Tarnopolski, Roberta Del Vecchio. "Gamma Ray Burst Prompt correlations." arXiv:1612.00618 (2016). https://pith.science/paper/DV5NO5AX
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-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,862 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.34 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.58 · compares with prior results 0.09 · mentions code or data availability 0.02.

The abstract, sentence by sentence

arXiv listing abstract v4. Results and the main claim are underlined; .

The mechanism responsible for the prompt emission of gamma-ray bursts (GRBs) is still a debated issue. The prompt phase-related GRB correlations can allow to discriminate among the most plausible theoretical models explaining this emission. We present an overview of the observational two-parameter correlations, their physical interpretations, their use as redshift estimators and possibly as cosmological tools. The nowadays challenge is to make GRBs, the farthest stellar-scaled objects observed (up to redshift $z=9.4$), standard candles through well established and robust correlations. However, GRBs spanning several orders of magnitude in their energetics are far from being standard candles. We describe the advances in the prompt correlation research in the past decades, with particular focus paid to the discoveries in the last 20 years.

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 The mechanism responsible for the prompt emission of gamma-ray bursts (GRBs) is still a debated issue. background 0.92 0.03 0.03 asserted 0.97
s1 The prompt phase-related GRB correlations can allow to discriminate among the most plausible theoretical models explaining this emission. background 0.95 0.05 0.13 hedged possibility 0.57
s2 We present an overview of the observational two-parameter correlations, their physical interpretations, their use as redshift estimators and possibly as cosmological tools. contribution 0.99 0.26 0.11 asserted 0.47
s3 The nowadays challenge is to make GRBs, the farthest stellar-scaled objects observed (up to redshift $z=9.4$), standard candles through well established and robust correlations. background 0.57 0.06 0.15 asserted 0.92
s4 However, GRBs spanning several orders of magnitude in their energetics are far from being standard candles. background 0.65 0.10 0.14 asserted 1.00
s5 We describe the advances in the prompt correlation research in the past decades, with particular focus paid to the discoveries in the last 20 years. contribution 0.93 0.22 0.05 asserted 0.78

What kind of paper the classifier reports this is: review 1.00 · evidence from literature 0.98.

What was examined, and what was not

sources read
  • arXiv listing abstract v4
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

The mechanism responsible for the prompt emission of gamma-ray bursts (GRBs) is still a debated issue. The prompt phase-related GRB correlations can allow to discriminate among the most plausible theoretical models explaining this emission. We present an overview of the observational two-parameter correlations, their physical interpretations, their use as redshift estimators and possibly as cosmological tools. The nowadays challenge is to make GRBs, the farthest stellar-scaled objects observed (up to redshift $z=9.4$), standard candles through well established and robust correlations. However, GRBs spanning several orders of magnitude in their energetics are far from being standard candles. We describe the advances in the prompt correlation research in the past decades, with particular focus paid to the discoveries in the last 20 years.

Human review

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

References
How the literature uses it

7 arXiv papers cite this in 7 sentences

Each citing sentence is taken from the citing paper's LaTeX source and typed by Pith's classifier. A label appears at probability 0.8 or more (0.95 for support), a contest at 0.7 or more; the quoted words are the citing authors'. How each label was checked · JSON

Papers citing it · 3 sentences without a confident label

Cites it as background 4 papers

Discussion

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