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Towards a Molecular Inventory of Protostellar Discs

Astrophysics · Submitted 27 Nov 2003

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

The authors' main claim The chemical environment in circumstellar discs is a unique diagnostic of the thermal, physical and chemical environment.

how it is stated · asserted 1.00 read the record →

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arXiv IDastro-ph/0311597 (version 1)
Pith ID4TN4LJPV, Pith's permanent record of this paper and its review
CitationC.V. Malcolm Fridlund, Glenn J White, Mark A. Thompson, Monica Huldtgren White. "Towards a Molecular Inventory of Protostellar Discs." arXiv:astro-ph/0311597 (2003). https://pith.science/paper/4TN4LJPV
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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, 2,257 input tokens.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.04 · human participants 0.01 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.04 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

The chemical environment in circumstellar discs is a unique diagnostic of the thermal, physical and chemical environment. In this paper we examine the structure of star formation regions giving rise to low mass stars, and the chemical environment inside them, and the circumstellar discs around the developing stars.

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 chemical environment in circumstellar discs is a unique diagnostic of the thermal, physical and chemical environment. background 1.00 0.06 0.08 asserted 1.00
s1 In this paper we examine the structure of star formation regions giving rise to low mass stars, and the chemical environment inside them, and the circumstellar discs around the developing stars. contribution 1.00 0.67 0.07 asserted 0.77

What kind of paper the classifier reports this is: review 0.42 · evidence from argument 0.76.

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
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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

The chemical environment in circumstellar discs is a unique diagnostic of the thermal, physical and chemical environment. In this paper we examine the structure of star formation regions giving rise to low mass stars, and the chemical environment inside them, and the circumstellar discs around the developing stars.

Human review

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