2019
DOI: 10.1103/physreve.99.052304
|View full text |Cite
|
Sign up to set email alerts
|

Sampling networks by nodal attributes

Abstract: In a social network individuals or nodes connect to other nodes by choosing one of the channels of communication at a time to re-establish the existing social links. Since available data sets are usually restricted to a limited number of channels or layers, these autonomous decision making processes by the nodes constitute the sampling of a multiplex network leading to just one (though very important) example of sampling bias caused by the behavior of the nodes. We develop a general setting to get insight and … Show more

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
2
1

Citation Types

2
25
0

Year Published

2019
2019
2024
2024

Publication Types

Select...
7
1

Relationship

0
8

Authors

Journals

citations
Cited by 18 publications
(27 citation statements)
references
References 30 publications
2
25
0
Order By: Relevance
“…It is also possible that the injection rate of accelerated protons is simultaneously enhanced. As a result, many models predict that the neutrino luminosity, L ν , is strongly enhanced during flares, with L ν ∝ L α γ , where L γ is the photon luminosity and α ∼ 1.5 − 2 Tavecchio et al 2014;Murase & Waxman 2016). From the experimental point of view, flares constitute ideal periods for neutrino emission, as the rate of background (atmospheric) neutrinos is reduced by focusing searches on a narrow time window.…”
Section: Introductionmentioning
confidence: 99%
“…It is also possible that the injection rate of accelerated protons is simultaneously enhanced. As a result, many models predict that the neutrino luminosity, L ν , is strongly enhanced during flares, with L ν ∝ L α γ , where L γ is the photon luminosity and α ∼ 1.5 − 2 Tavecchio et al 2014;Murase & Waxman 2016). From the experimental point of view, flares constitute ideal periods for neutrino emission, as the rate of background (atmospheric) neutrinos is reduced by focusing searches on a narrow time window.…”
Section: Introductionmentioning
confidence: 99%
“…Firstly, neutrinos can be preferentially produced during γ-ray flares as typically, in models where the majority of γ-rays are leptonic in origin, L ν ∝ L γ rad , with γ ∼ 1.5 − 2.0. This was demonstrated, for example, in [6,24,25] and references therein. Therefore,…”
Section: Contribution From Blazar Flares: Duty Cycle and Neutrino Enhmentioning
confidence: 75%
“…The absence of high-energy multiplets in the IceCube data can be used to constrain the number density of sources contributing to the diffuse neutrino background [6,7] (see also earlier work by [8][9][10]). The IceCube diffuse flux,…”
Section: Blazar Contribution To the Diffuse Neutrino Flux 21 Clustermentioning
confidence: 99%
“…Our model for highenergy emissions from galaxy mergers connects the electromagnetic emissions from merging regions to the neutrino emission and CR acceleration. With the prospects for detecting or setting the limits on their high-energy neutrino emission by current and/or next-generation neutrino detectors (Murase & Waxman 2016;Yuan et al 2018), our work will be able to provide a new perspective on future multi-messenger studies of the evolution of galaxies.…”
Section: Summary and Discussionmentioning
confidence: 99%