Introducing the H-Index in Telescope Statistics
Astrophysics
2007-05-23 v1
Abstract
This paper analyzes the performance of observatories based on the so-called h-index (Hirsch 2005), a new, easy-to-use parameter that quantifies scientists' research impact and relevance. Compared to other bibliometric criteria, like total number of publications or citations, the h-index is less biased. Using NASA's Astrophysics Data System (ADS), we investigate the performance of selected observatories, taking into account their specific number of years of operation.
Cite
@article{arxiv.astro-ph/0610274,
title = {Introducing the H-Index in Telescope Statistics},
author = {Uta Grothkopf and Sarah Stevens-Rayburn},
journal= {arXiv preprint arXiv:astro-ph/0610274},
year = {2007}
}
Comments
7 pages, 4 figures, to appear in the proceedings of Library and Information Services in Astronomy V, Cambridge, MA, June 2006, S. Ricketts, E. Isaksson, C. Birdie (eds.)