Table 6.
Contaminants amongst z > 6 galaxies in the restricted faint mock sample.
| Filters | True z > 6 | Contaminants | Contamination fraction | Completeness |
|---|---|---|---|---|
| Euclid | 609 | 204 |
 |
91% |
| Euclid + Rubin | 609 | 202 |
 |
91% |
| Euclid + Rubin DDF | 636 | 28 |
 |
95% |
| Euclid + H20 | 617 | 172 |
 |
92% |
| Euclid + Spitzer | 312 | 107 |
 |
91% |
| Euclid + Rubin + Spitzer | 315 | 97 |
 |
92% |
| Euclid + Rubin DDF + Spitzer | 329 | 18 |
 |
96% |
| Euclid + H20 + Spitzer | 309 | 94 |
 |
90% |
Notes. Number of true z > 6 galaxies and z > 6 contaminants, from various combinations of Euclid and ancillary data, based on the restricted faint mock sample. The restricted faint mock sample consists of sources that have a 5σ flux measurement in at least one the Euclid NIR bands. We report the contamination fraction and z > 6 completeness, where the latter is calculated as the fraction of all fiducial zfid = 6–8 sources that satisfy the detection threshold requirement.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.