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CO on Titan: More Evidence for a Well-Mixed Vertical Profile

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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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M.A. Gurwell (Harvard-Smithsonian Center for Astrophysics), D.O. Muhleman (Division of Geological, Planetary Sciences, Caltech)

Astrophysics · Submitted 16 Feb 2000

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

The authors' main claim We find that the spectrum is best fit by a uniform profile of 52 ppm, with estimated errors of 6 ppm (40 to 200 km) and 12 ppm (200 to 300 km).

how it is stated · asserted 1.00 read the record →

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arXiv IDastro-ph/0002331 (version 1)
Pith IDWFPBOCCY, Pith's permanent record of this paper and its review
CitationCaltech), D.O. Muhleman (Division of Geological, M.A. Gurwell (Harvard-Smithsonian Center for Astrophysics), Planetary Sciences. "CO on Titan: More Evidence for a Well-Mixed Vertical Profile." arXiv:astro-ph/0002331 (2000). https://pith.science/paper/WFPBOCCY
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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, 2,299 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.49 · human participants 0.01 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.99 · compares with prior results 0.10 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We report new interferometric observations of the CO (2-1) rotational transition on Titan. We find that the spectrum is best fit by a uniform profile of 52 ppm, with estimated errors of 6 ppm (40 to 200 km) and 12 ppm (200 to 300 km).

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 report new interferometric observations of the CO (2-1) rotational transition on Titan. contribution 0.95 0.96 0.03 asserted 0.91
s1 We find that the spectrum is best fit by a uniform profile of 52 ppm, with estimated errors of 6 ppm (40 to 200 km) and 12 ppm (200 to 300 km). result 1.00 0.97 0.85 asserted 1.00

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

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 report new interferometric observations of the CO (2-1) rotational transition on Titan. We find that the spectrum is best fit by a uniform profile of 52 ppm, with estimated errors of 6 ppm (40 to 200 km) and 12 ppm (200 to 300 km).

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