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A Search for Radio-loud Quasars within the Epoch of Reionization

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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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Matt J.Jarvis (1), Steve Rawlings (1), F.Eugenio Barrio (1), Gary J.Hill (2), Amanda Bauer (2), Steve Croft (3) ((1) Oxford University, (2) University of Austin at Texas, (3) Lawrence Livermore National Laboratory)

Astrophysics · Submitted 15 Sep 2003

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

The authors' main claim In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5.

how it is stated · asserted 0.98 read the record →

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arXiv IDastro-ph/0309379 (version 1)
Pith IDAWMNGLCS, Pith's permanent record of this paper and its review
Citation(2) University of Austin at Texas, (3) Lawrence Livermore National Laboratory), Amanda Bauer (2), F.Eugenio Barrio (1), Gary J.Hill (2), Matt J.Jarvis (1), Steve Croft (3) ((1) Oxford University, Steve Rawlings (1). "A Search for Radio-loud Quasars within the Epoch of Reionization." arXiv:astro-ph/0309379 (2003). https://pith.science/paper/AWMNGLCS
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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-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,963 input tokens.

What the abstract itself states, as probabilities: claims first 0.21 · states limitation 0.28 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.10 · compares with prior results 0.09 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

The Universe became fully reionized, and observable optically, at a time corresponding to redshift z~6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formation. At present no targets for such studies are known. In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5.

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 Universe became fully reionized, and observable optically, at a time corresponding to redshift z~6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formation. background 1.00 0.05 0.08 asserted 0.94
s1 At present no targets for such studies are known. gap 1.00 0.21 0.06 asserted 1.00
s2 In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5. contribution 0.99 0.80 0.12 asserted 0.98

What kind of paper the classifier reports this is: position or commentary 0.84 · evidence from observation or experiment 0.57.

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

The Universe became fully reionized, and observable optically, at a time corresponding to redshift z~6.5, so it is only by studying the HI and molecular absorption lines against higher-redshift, radio-loud sources that one can hope to make detailed studies of the earliest stages of galaxy formation. At present no targets for such studies are known. In these proceedings we describe a survey which is underway to find radio-loud quasars at z > 6.5.

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