Bibliometric indicators of young authors in astrophysics: Can later stars be predicted?

被引:18
作者
Havemann, Frank [1 ]
Larsen, Birger [2 ]
机构
[1] Humboldt Univ, Inst Bibliotheks & Informat Wissensch, D-10099 Berlin, Germany
[2] Aalborg Univ, Dept Commun, Copenhagen, Denmark
关键词
Bibliometric indicators; Research evaluation; Astrophysics; Citation analysis; Performance of young authors; Comparison of indicators; CITATION IMPACT; H-INDEX; SCIENTIFIC PERFORMANCE; OUTPUT; SCIENCE; SCORE;
D O I
10.1007/s11192-014-1476-3
中图分类号
TP39 [计算机的应用];
学科分类号
081203 ; 0835 ;
摘要
We test 16 bibliometric indicators with respect to their validity at the level of the individual researcher by estimating their power to predict later successful researchers. We compare the indicators of a sample of astrophysics researchers who later co-authored highly cited papers before their first landmark paper with the distributions of these indicators over a random control group of young authors in astronomy and astrophysics. We find that field and citation-window normalisation substantially improves the predicting power of citation indicators. The sum of citation numbers normalised with expected citation numbers is the only indicator which shows differences between later stars and random authors significant on a 1 % level. Indicators of paper output are not very useful to predict later stars. The famous h-index makes no difference at all between later stars and the random control group.
引用
收藏
页码:1413 / 1434
页数:22
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