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Table 2
Quality of the photo-z retrieved for a subsample of RS galaxies in ALHAMBRA, when different method are applied: our code alone, BPZ2.0, EAZY, and our code using BPZ2.0 and EAZY as input values of redshift.
| σ NMAD | σz/ (1 + zs) | η 1 | η 2 | |
|
|
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| MUFFIT | 0.0157 | 0.0105 | 1.6% | 5.8% |
| BPZ2.0 | 0.0104 | 0.0076 | 0.9% | 7.7% |
| EAZY | 0.0102 | 0.0083 | 0.8% | 4.0% |
|
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| MUFFIT + BPZ2.0 | 0.0087 | 0.0070 | 0.9% | 6.3% |
| MUFFIT + EAZY | 0.0092 | 0.0071 | 0.7% | 5.5% |
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