Measuring the transition to homogeneity with photometric redshift surveys
We study the possibility of detecting the transition to homogeneity using photometric redshift catalogues. Our method is based on measuring the fractality of the projected galaxy distribution, using angular distances, and relies only on observable quantities. It thus provides a way to test the cosmo...
| 主要な著者: | , , , , |
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| フォーマット: | Journal article |
| 出版事項: |
Oxford University Press
2014
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