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...
| Hoofdauteurs: | , , , , |
|---|---|
| Formaat: | Journal article |
| Gepubliceerd in: |
Oxford University Press
2014
|