2016
DOI: 10.1016/j.joi.2016.04.009
|View full text |Cite
|
Sign up to set email alerts
|

Gazing at the skyline for star scientists

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

0
9
0

Year Published

2017
2017
2024
2024

Publication Types

Select...
7
3

Relationship

0
10

Authors

Journals

citations
Cited by 26 publications
(10 citation statements)
references
References 51 publications
0
9
0
Order By: Relevance
“…Since Spearman coefficient (ρ) is independent of the normality of the data distribution and moreover it can handle ties, in this study has been used Spearman ρ coefficient for the construction of the correlation matrix. 41,9 The correlation matrix (12×12) was formulated and most indicators were found to be significantly correlated (Spearman ρ > 0.8) with each other at a statistical significance level of 0.05, but there were also a few indicators that showed no strong correlation (ρ < 0.5) with the majority of other indicators. Table 5 shows that, the Spearman's ρ correlation coefficient between JCRIF and AIF (after removing self-citations) reaches a statistical significance level with a high correlation, ρ = 0.96.…”
Section: Discussionmentioning
confidence: 99%
“…Since Spearman coefficient (ρ) is independent of the normality of the data distribution and moreover it can handle ties, in this study has been used Spearman ρ coefficient for the construction of the correlation matrix. 41,9 The correlation matrix (12×12) was formulated and most indicators were found to be significantly correlated (Spearman ρ > 0.8) with each other at a statistical significance level of 0.05, but there were also a few indicators that showed no strong correlation (ρ < 0.5) with the majority of other indicators. Table 5 shows that, the Spearman's ρ correlation coefficient between JCRIF and AIF (after removing self-citations) reaches a statistical significance level with a high correlation, ρ = 0.96.…”
Section: Discussionmentioning
confidence: 99%
“…Methods for determining the characteristics of top performers proliferate, and they are studied as individual scientists or scientists embedded in organizational contexts, with reciprocal relationships: how they influence and how they are influenced by their organizations or collaborative networks. The skyline for star scientists (Sidiropoulos et al 2016 ) is being sought: stars are those scientists whose performance cannot be surpassed by others with respect to all scientometric indexes selected. Apart from stars, the relevant studies focus on the scientific elite or the most highly cited scientists (Parker et al 2010 , 2013 ), top researchers (Abramo et al 2013 ; Cortés et al 2016 ), the academic elite (Yin and Zhi 2017 ), or prolific professors (Piro et al 2016 ).…”
Section: Theoretical Frameworkmentioning
confidence: 99%
“…Given the high correlation amongst bibliometric performance metrics and based on proposed categorizations of those metrics in [10], [36], we opted for three straightforward "raw" metrics to represent both impact and productivity (feature set F 1): citation count (c) to represent cumulative impact, h-index (h) for ranked output, and citation rate (c/p, where p is the number of publications) to account for impact normalized over productivity. Figure 2 depicts the coefficient of variation (βCV ) [37] for various contemplated combinations of features and number of clusters k. When βCV curve stabilizes, it is expected that the variabilities in the intra and inter-cluster distances remain stable, implying that adding more clusters should be of little help to understand the dataset variability.…”
Section: Defining Clusters Of Peersmentioning
confidence: 99%