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Table E.2.
Redshift prediction performance for HIEROs obtained considering Rubin depths after one and four years of observations.
| Rubin year | N | RMSE | OLF | NMAD | ⟨Δz⟩ |
|---|---|---|---|---|---|
| 1 | 115 303 | 0.864 | 0.301 | 0.112 | −0.064 |
| 4 | 115 371 | 0.858 | 0.229 | 0.110 | −0.031 |
| 10 | 184 441 | 0.654 | 0.123 | 0.068 | −0.084 |
Notes.N indicates the number of objects in the selection. For ease of comparison, we report again the results after 10 years of Rubin observations, already presented in Table 5.
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