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Constraints on stellar parameters of the SPB star HD182255 from complex asteroseismology

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Przemys{l}aw Walczak, Wojciech Szewczuk, Jadwiga Daszyńska-Daszkiewicz

Solar and Stellar Astrophysics · Submitted 19 Dec 2012

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

The authors' main claim Seismic modeling of the Slowly Pulsating B-type star HD182255 yields strong constraints on the radial orders of the two dominant modes.

how it is stated · asserted 1.00 read the record →

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arXiv ID1212.4643 (version 1)
Pith IDXIZLHUEJ, Pith's permanent record of this paper and its review
CitationJadwiga Daszy\'nska-Daszkiewicz, Przemys{\l}aw Walczak, Wojciech Szewczuk. "Constraints on stellar parameters of the SPB star HD182255 from complex asteroseismology." arXiv:1212.4643 (2012). https://pith.science/paper/XIZLHUEJ
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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-1.13-20260917 via OpenRouter, question bank abstract-p1-20260923, 2026-09-23: 1 request, 2,939 input tokens, $0.0001 reported.

What the abstract itself states, as probabilities: claims first 0.03 · states limitation 0.08 · human participants 0.01 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.24 · compares with prior results 0.20 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

Seismic modeling of the Slowly Pulsating B-type star HD182255 yields strong constraints on the radial orders of the two dominant modes. For these frequencies, we derive also the empirical values of the complex nonadiabatic parameter $f$. These two seismic tools, i.e., pulsational frequencies and the associated values of $f$, allow to test available opacity data, chemical composition and overshooting efficiency.

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 Seismic modeling of the Slowly Pulsating B-type star HD182255 yields strong constraints on the radial orders of the two dominant modes. result 0.88 0.91 0.58 asserted 1.00
s1 For these frequencies, we derive also the empirical values of the complex nonadiabatic parameter $f$. result 0.98 0.95 0.09 asserted 1.00
s2 These two seismic tools, i.e., pulsational frequencies and the associated values of $f$, allow to test available opacity data, chemical composition and overshooting efficiency. interpretation 0.89 0.47 0.37 asserted 0.76

What kind of paper the classifier reports this is: empirical study 0.66 · evidence from analysis of existing data 0.53.

What was examined, and what was not

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  • arXiv listing abstract v1
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  • 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
  • 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

Seismic modeling of the Slowly Pulsating B-type star HD182255 yields strong constraints on the radial orders of the two dominant modes. For these frequencies, we derive also the empirical values of the complex nonadiabatic parameter $f$. These two seismic tools, i.e., pulsational frequencies and the associated values of $f$, allow to test available opacity data, chemical composition and overshooting efficiency.

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