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Tabular Foundation Models for the Estimation of Probabilistic Quasar Photometric Redshifts in S-PLUS

  • Authors: Raquel R. Valença, Lilianne Nakazono, Rafael Izbicki, Marco Henrique de Almeida Inácio, Bruno Marcondes e Resende, Maycon Jorge Deláqua da Silva, Kiana Coimbra Buin Lins, Natanael M. Cardoso, Claudia Mendes de Oliveira

Raquel R. Valença et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 3.

Per-redshift-bin RMSE and η0.15 on the DR6 test set at ntrain = 121,626 for the three methods with the lowest overall unweighted RMSE in Table 3 (top panel): TabPFN 2.5, MDN-deep, and GBM-Point. Bins have the fixed width Δzspec = 0.5; bins with fewer than 30 test objects are dropped. Shaded bands are ±1 SE. All three methods agree to within one SE in the midredshift range zspec ∈ [0.5, 3.0]; differences are concentrated at the low- and high-z ends, where the foundation method performs the best.

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