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Isolated Neutron Stars

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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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V. M. Kaspi, M. S. E. Roberts (McGill), A. K. Harding (GSFC)

Astrophysics · Submitted 5 Feb 2004

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

The authors' main claim This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars.

how it is stated · asserted 0.91 read the record →

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arXiv IDastro-ph/0402136 (version 2)
Pith IDG6DJ6F3W, Pith's permanent record of this paper and its review
CitationA. K. Harding (GSFC), M. S. E. Roberts (McGill), V. M. Kaspi. "Isolated Neutron Stars." arXiv:astro-ph/0402136 (2004). https://pith.science/paper/G6DJ6F3W
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, 2,214 input tokens.

What the abstract itself states, as probabilities: claims first 0.02 · states limitation 0.11 · human participants 0.02 · controlled comparison 0.02 · randomized assignment 0.01 · states quantitative result 0.03 · compares with prior results 0.04 · mentions code or data availability 0.01.

The abstract, sentence by sentence

arXiv listing abstract v2. Results and the main claim are underlined; .

This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae.

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 This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. contribution 0.94 0.15 0.07 asserted 0.91
s1 Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae. contribution 0.84 0.06 0.04 asserted 0.73

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

What was examined, and what was not

sources read
  • arXiv listing abstract v2
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

This is a review of X-ray emission from all types of isolated neutron stars, with an emphasis on rotation-powered pulsars. Topics include magnetospheric and thermal emission, as well as pulsar wind nebulae.

Human review

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

References
How the literature uses it

2 arXiv papers cite this in 2 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

Discussion

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