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HI Study of Southern Galactic Supernova Remnants

Astrophysics · Submitted 6 Nov 2003

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

The authors' main claim For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results.

how it is stated · unclear 0.69 read the record →

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arXiv IDastro-ph/0311144 (version 1)
Pith IDEMPZOUDF, Pith's permanent record of this paper and its review
CitationBon-Chul Koo, Ji-hyun Kang, Naomi McClure-Griffiths. "HI Study of Southern Galactic Supernova Remnants." arXiv:astro-ph/0311144 (2003). https://pith.science/paper/EMPZOUDF
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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, 2,272 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.15 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.06 · 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; .

We briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results.

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 briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. contribution 0.93 0.80 0.07 asserted 0.65
s1 For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results. contribution 0.55 0.77 0.10 unclear 0.69

What kind of paper the classifier reports this is: empirical study 0.70 · evidence from observation or experiment 0.67.

What was examined, and what was not

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  • references and citing sentences
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  • P abstract
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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 briefly summarize the survey of HI 21 cm emission lines to search for shocked atomic gas associated with Galactic supernova remnants (SNRs) in the southern sky. For G347.3-0.5, we discuss the distance to the SNR and the implications of the HI results.

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