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| Main Authors: | , |
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| Format: | Preprint |
| Published: |
2025
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| Subjects: | |
| Online Access: | https://arxiv.org/abs/2505.09234 |
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| _version_ | 1866915287160324096 |
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| author | Chambon, Hugo Fraix-Burnet, Didier |
| author_facet | Chambon, Hugo Fraix-Burnet, Didier |
| contents | An automatic procedure to perform sub-clustering on large samples is presented. At each iteration, the most diverse cluster is sub-clustered, and the global diversity of the new classification is compared to the previous one. The process stops if no improvement is found. The key to our procedure is the use of a quantitative measure of diversity, called the Leinster-Cobbold index, that takes into account the similarity between clusters. While this procedure has been successfully applied on a large sample of spectra of galaxies, we illustrate its efficiency with two examples in this paper. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2505_09234 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | The Leinster-Cobbold diversity index as a criterion for sub-clustering Chambon, Hugo Fraix-Burnet, Didier Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics An automatic procedure to perform sub-clustering on large samples is presented. At each iteration, the most diverse cluster is sub-clustered, and the global diversity of the new classification is compared to the previous one. The process stops if no improvement is found. The key to our procedure is the use of a quantitative measure of diversity, called the Leinster-Cobbold index, that takes into account the similarity between clusters. While this procedure has been successfully applied on a large sample of spectra of galaxies, we illustrate its efficiency with two examples in this paper. |
| title | The Leinster-Cobbold diversity index as a criterion for sub-clustering |
| topic | Instrumentation and Methods for Astrophysics Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2505.09234 |