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Table 1
Absolute residuals (|γ|) between the measured ALMA flux densities and the fluxes of the best fitting SEDs at the ALMA wavelengths expressed as a multiple of the error on the ALMA flux density.
| |γ| | Flat prior | Informed prior |
|
|
||
| 1 | 77 (36.2%) | 98 (46.0%) |
| 2 | 121 (56.8%) | 142 (66.7%) |
| 3 | 146 (68.5%) | 166 (77.9%) |
| 4 | 160 (75.1%) | 184 (86.4%) |
| 5 | 177 (83.1%) | 192 (90.1%) |
Notes. The values in Cols. 2 and 3 are the number (percentage) of objects with a |γ| less than the value in Col. 1.
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