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Introducing the H-Index in Telescope Statistics

Uta Grothkopf·Sarah Stevens-Rayburn
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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.

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Uta Grothkopf, Sarah Stevens-Rayburn. 2006-10-10. Introducing the H-Index in Telescope Statistics. https://arxiv.org/abs/astro-ph/0610274

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