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Recurrence plots of pulsar profiles

descriptionPublicationkeyboard_double_arrow_right Article 01 Jan 2015 Italy English Publisher:Zenodo
Authors: SPARAVIGNA, Amelia Carolina;

doi: 10.5281/zenodo.3908959 , 10.5281/zenodo.3908958

handle: 11583/2620134

Recurrence plots of pulsar profiles

Abstract

Pulsars are rotating neutron stars that have an emission of electromagnetic radiations which is continuous but beamed. Therefore, an observer sees a pulse of radiation when the beam sweeps across his line-of-sight. Averaging over many pulses, a pulse profile specific for the observed pulsar is obtained. Here we propose the use of a recurrence plot for showing it. This plot can highlight specific behaviours in pulse profiles.

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Recurrence Plots, Pulse Profiles., [SDU.ASTR.SR] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR], Recurrence Plots; Pulsars; Pulse Profiles, Pulsars, Pulse Profiles

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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