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Table 5.

MDN performance evaluation.

IGMM implementation Photometry ⟨Δz⟩ (zs < 1) rms(Δz) (zs < 1) ⟨Δz⟩, range1 (a)
Fully unsup. griz, W1, W2 0.0007 ± 0.0006 0.0204 ± 0.0106 0.0025 ± 0.0005
Spec. class griz, W1, W2 0.0030 ± 0.0028 0.0216 ± 0.0104 0.0042 ± 0.039
Redshift (zs) griz, W1, W2 0.0022 ± 0.0024 0.0207 ± 0.0113 0.0008 ± 0.0003
Spec. class, zs griz, W1, W2 0.0001 ± 0.0005 0.0208 ± 0.0112 0.0058 ± 0.0006
Spec. class ugriz, W1, W2 0.0023 ± 0.0026 0.0181 ± 0.0091 0.0004 ± 0.0025

IGMM implementation photometry rms(Δz), range1 (a) rms(Δz), range2 (b) rms(Δz), range3 (c)

Fully unsup. griz, W1, W2 0.0215 ± 0.0013 0.0233 ± 0.0013 0.0238 ± 0.0015
Spec. class griz, W1, W2 0.0230 ± 0.0015 0.0245 ± 0.0019 0.0247 ± 0.0014
Redshift (zs) griz, W1, W2 0.0219 ± 0.0014 0.0238 ± 0.0012 0.0242 ± 0.0013
Spec. class, zs griz, W1, W2 0.0218 ± 0.0019 0.0235 ± 0.0019 0.0235 ± 0.0024
Spec. class ugriz, W1, W2 0.0179 ± 0.0015 0.0182 ± 0.0016 0.0187 ± 0.0019

Notes. The bias and rms are computed using the definition of clipped bias and rms in PS1-STR (Beck et al. 2021).

(a)

Restricted to galaxies with zs < 0.3;

(b)

restricted to galaxies with zs < 0.4;

(c)

restricted to galaxies with zs < 0.5.

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