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One Hundred Years of Observations of the Be Star HDE 245770 (the X-ray Binary A0535+26/V725 Tau): The End of an Active Phase

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V.M. Lyuty, G.V. Zaitseva (Sternberg Astronomical Institute, Moscow)

Astrophysics · Submitted 21 Jul 2000

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

The authors' main claim Based on our and published data, we analyze the photometric history of the star from 1898.

how it is stated · asserted 0.98 read the record →

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arXiv IDastro-ph/0007321 (version 1)
Pith IDCV53UBVA, Pith's permanent record of this paper and its review
CitationG.V. Zaitseva (Sternberg Astronomical Institute, Moscow), V.M. Lyuty. "One Hundred Years of Observations of the Be Star HDE 245770 (the X-ray Binary A0535+26/V725 Tau): The End of an Active Phase." arXiv:astro-ph/0007321 (2000). https://pith.science/paper/CV53UBVA
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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, 2,340 input tokens.

What the abstract itself states, as probabilities: claims first 0.04 · states limitation 0.09 · human participants 0.02 · controlled comparison 0.04 · randomized assignment 0.01 · states quantitative result 0.24 · compares with prior results 0.60 · mentions code or data availability 0.03.

The abstract, sentence by sentence

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

UBV observations of the X-ray binary system A0535+26/V725 Tau at the Crimean Station of the Sternberg Astronomical Institute in 1980-1998 are presented. Based on our and published data, we analyze the photometric history of the star from 1898.

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 UBV observations of the X-ray binary system A0535+26/V725 Tau at the Crimean Station of the Sternberg Astronomical Institute in 1980-1998 are presented. contribution 0.78 0.92 0.04 asserted 0.99
s1 Based on our and published data, we analyze the photometric history of the star from 1898. contribution 0.66 0.68 0.09 asserted 0.98

What kind of paper the classifier reports this is: empirical study 1.00 · evidence from observation or experiment 0.77.

What was examined, and what was not

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  • figures and tables
  • references and citing sentences
  • relations to other papers
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  • P abstract
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  • T body sentences
  • C citations
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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

UBV observations of the X-ray binary system A0535+26/V725 Tau at the Crimean Station of the Sternberg Astronomical Institute in 1980-1998 are presented. Based on our and published data, we analyze the photometric history of the star from 1898.

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