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Table 4
Comparison of stellar mass estimates between our catalog and reference catalogs.
catalog | N | Δ | NMAD | r | err |
---|---|---|---|---|---|
COSMOS2020(FARMER) | 1899 | 0.001 | 0.176 | 0.96 | 0.132 |
COSMOS2020(CLASSIC) | 2485 | −0.014 | 0.156 | 0.97 | 0.125 |
DEVILS | 5080 | −0.100 | 0.207 | 0.82 | 0.142 |
SDSS(Firefly) | 24 947 | 0.060 | 0.321 | 0.85 | 0.097 |
SDSS(MPA-JHU) | 18 778 | −0.071 | 0.126 | 0.98 | 0.100 |
GSWLC | 17 902 | −0.191 | 0.284 | 0.97 | 0.100 |
Zou et al. (2024) | 761 096 | −0.105 | 0.173 | 0.98 | 0.120 |
FastSpecFit 3.2 | 1 121 332 | −0.318 | 0.503 | 0.85 | 0.156 |
PROVABGS | 215 123 | −0.393 | 0.582 | 0.89 | 0.116 |
Notes. The median difference (Δ), NMAD and Pearson coefficient (r; see Sect. 5.1 for definitions), and the median error of stellar masses (err) for the given sample (with a N number of sources) are provided.
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