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Table 4

Summary of the results in the different configurations tested in this work depending on i-band cuts.

Sample Bands Weighted mi < 22.5 mi < 24 mi < 25 mi < 26 mi < 27
σ η σ η σ η σ η σ η
hscPipe/Phosphoros
Spec-z NIR 0.025 1.6% 0.026 2.3% 0.027 3.1% 0.028 3.4% –
Spec-z NIR Yes 0.025 1.6% 0.026 3.0% 0.034 6.0% 0.044 9.9% –
Spec-z Ugrizy 0.036 2.1% 0.037 3.3% 0.037 4.2% 0.038 4.7% –
Spec-z Ugrizy Yes 0.036 2.1% 0.037 4.3% 0.042 9.6% 0.057 16.1% –
C 20 F/E NIR 0.030 6.8% 0.030 6.8% 0.035 8.3% 0.045 12.2% 0.063 20.5%
C 20 F/E Ugrizy 0.036 8.0% 0.038 9.4% 0.044 12.6% 0.055 17.1% 0.079 25.8%
SExtractor/LePhare
Spec-z NIR 0.023 1.2% 0.024 1.9% 0.025 2.5% 0.026 2.9% –
Spec-z NIR Yes 0.023 1.2% 0.025 2.5% 0.028 5.1% 0.035 9.5% –
Spec-z Ugrizy 0.027 2.1% 0.027 3.2% 0.028 4.0% 0.028 4.4% –
Spec-z Ugrizy Yes 0.027 2.1% 0.027 4.2% 0.033 8.4% 0.049 17.2% –
C 20 F/E NIR 0.025 6.5% 0.027 5.8% 0.030 6.5% 0.036 9.0% 0.049 16.3%
C 20 F/E Ugrizy 0.026 6.9% 0.028 6.8% 0.034 8.5% 0.042 11.7% 0.060 20.7%

Notes. The weighted column indicates if the results on the spectroscopic sample are weighted by the number of photometric sources (see Eqs. (8) and (9)). C 20 F/E are the COSMOS2020 FARMER/EAzY photo-zs.

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