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Revisiting a non-parametric reconstruction of the deceleration parameter from observational data

descriptionPublicationkeyboard_double_arrow_right Article 30 Jul 2020Publisher:Zenodo
Authors: Purba Mukherjee; Narayan Banerjee;

doi: 10.5281/zenodo.3967607 , 10.5281/zenodo.3967606 , 10.5281/zenodo.4412042

Revisiting a non-parametric reconstruction of the deceleration parameter from observational data

Abstract

This .zip file contains a compilation of the source observational data, and deceleration parameter data set generated on performing the model-independent reconstruction, using Gaussian Process Methodology.

Related Organizations
Keywords

reconstruction, deceleration parameter, dark energy, cosmology

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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.
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