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Dynamical properties of binary stars hosting planets in the Galactic Center

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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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Nazanin Davari, Roberto Capuzzo-Dolcetta

Astrophysics of Galaxies · Submitted 9 Jun 2019

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

The authors' main claim We present some preliminary results of our work about the close encounter of binary stars hosting planets on S-type orbits with the Sgr A* supermassive black hole in the center of our Galaxy.

how it is stated · asserted 0.75 read the record →

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arXiv ID1906.03738 (version 1)
Pith IDD3BQRN4Z, Pith's permanent record of this paper and its review
CitationNazanin Davari, Roberto Capuzzo-Dolcetta. "Dynamical properties of binary stars hosting planets in the Galactic Center." arXiv:1906.03738 (2019). https://pith.science/paper/D3BQRN4Z
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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, 1,633 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.78 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.04 · compares with prior results 0.05 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

We present some preliminary results of our work about the close encounter of binary stars hosting planets on S-type orbits with the Sgr A* supermassive black hole in the center of our Galaxy.

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 present some preliminary results of our work about the close encounter of binary stars hosting planets on S-type orbits with the Sgr A* supermassive black hole in the center of our Galaxy. contribution 1.00 0.81 0.08 asserted 0.75

What kind of paper the classifier reports this is: simulation study 0.97 · evidence from simulation or computation 0.96.

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 present some preliminary results of our work about the close encounter of binary stars hosting planets on S-type orbits with the Sgr A* supermassive black hole in the center of our Galaxy.

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