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A very rapid Extreme Scattering Event in the IDV source 0954+658

Astrophysics · Submitted 24 Oct 2001

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

The authors' main claim During an Intraday Variability (IDV) monitoring project (March 2000), a feature resembling an ESE-like event appeared in the variable light curve of 0954+658, however with a time scale of less than two days.

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arXiv IDastro-ph/0110527 (version 1)
Pith ID3ZZ26UC5, Pith's permanent record of this paper and its review
CitationA. Kraus, A. Witzel, Bonn), G. Cim\`o, J. A. Zensus (Max-Planck-Institut fuer Radioastronomie, L. Fuhrmann, T. Beckert, T. P. Krichbaum. "A very rapid Extreme Scattering Event in the IDV source 0954+658." arXiv:astro-ph/0110527 (2001). https://pith.science/paper/3ZZ26UC5
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Compiled by classifier-1.13.0 via TypeSafe API, question bank abstract-p1-20260923, 2026-09-23: 1 request, 4,912 input tokens.

What the abstract itself states, as probabilities: claims first 0.05 · states limitation 0.17 · human participants 0.02 · controlled comparison 0.03 · randomized assignment 0.01 · states quantitative result 0.91 · compares with prior results 0.72 · mentions code or data availability 0.02.

The abstract, sentence by sentence

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

Extreme Scattering Events (ESEs) are dramatic variations of the flux density at Gigahertz frequencies caused by ray path distortions within an isolated inhomogeneity ("plasma lens") in the interstellar medium. These events are characterized by a deep flux density minimum in the light curve with, in some cases, surrounding maxima. The variability time scales range from weeks to months. These phenomena show a strong frequency dependence, in which the variability amplitudes increase with wavelength. During an Intraday Variability (IDV) monitoring project (March 2000), a feature resembling an ESE-like event appeared in the variable light curve of 0954+658, however with a time scale of less than two days. We will discuss this effect and its implications for a better description of the interstellar medium.

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 Extreme Scattering Events (ESEs) are dramatic variations of the flux density at Gigahertz frequencies caused by ray path distortions within an isolated inhomogeneity ("plasma lens") in the interstellar medium. background 1.00 0.05 0.03 asserted 1.00
s1 These events are characterized by a deep flux density minimum in the light curve with, in some cases, surrounding maxima. background 1.00 0.06 0.03 asserted 0.93
s2 The variability time scales range from weeks to months. background 1.00 0.07 0.03 asserted 1.00
s3 These phenomena show a strong frequency dependence, in which the variability amplitudes increase with wavelength. background 1.00 0.09 0.04 asserted 1.00
s4 During an Intraday Variability (IDV) monitoring project (March 2000), a feature resembling an ESE-like event appeared in the variable light curve of 0954+658, however with a time scale of less than two days. result 0.96 0.95 0.34 asserted 0.93
s5 We will discuss this effect and its implications for a better description of the interstellar medium. future work 0.80 0.30 0.10 unclear 0.94

What kind of paper the classifier reports this is: empirical study 1.00 · evidence from observation or experiment 0.89.

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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

Extreme Scattering Events (ESEs) are dramatic variations of the flux density at Gigahertz frequencies caused by ray path distortions within an isolated inhomogeneity ("plasma lens") in the interstellar medium. These events are characterized by a deep flux density minimum in the light curve with, in some cases, surrounding maxima. The variability time scales range from weeks to months. These phenomena show a strong frequency dependence, in which the variability amplitudes increase with wavelength. During an Intraday Variability (IDV) monitoring project (March 2000), a feature resembling an ESE-like event appeared in the variable light curve of 0954+658, however with a time scale of less than two days. We will discuss this effect and its implications for a better description of the interstellar medium.

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