Open Access

Table C.1.

Data used to fit the SEDs.

ID Obs. frequency Flux Ref.
(GHz) (mJy)
AJ025-33 407 6.8 ± 0.7 This work (a)
342 4.7 ± 0.5 This work (b)
259 2.5 ± 0.3 (1)
192 1.1 ± 0.1 This work (b)
103 0.10 ± 0.02 This work (c)

J0305-3150 407 10.5 ± 1.5 This work (a)
336 9.7 ± 1.0 (2)
250 5.3 ± 0.6 (1)
99 0.23 ± 0.04 (3)

J0439+1634* 407 45.5 ± 4.7 This work (a)
353 26.2 ± 3.1 (4)
271 16.9 ± 1.7 (4)
255 15.5 ± 1.6 (4)
245 16.0 ± 1.6 (5)
239 14.0 ± 1.4 (4)
155 3.50 ± 0.4 (4)
139 2.70 ± 0.3 (4)
109 1.60 ± 0.2 (4)
93 1.30 ± 0.1 (4)

J2318-3029 407 6.9 ± 1.0 This work (a)
266 3.1 ± 0.3 (1)
106 0.26 ± 0.04 This work (c)

J2348-3054 670 9.1 ± 1.4 (6)
407 5.5 ± 0.7 This work (a)
240 2.28 ± 0.2 (1)
95 0.12 ± 0.02 (3)

PJ007+04 407 4.7 ± 0.6 This work (a)
271 2.33 ± 0.2 (1)
158 0.57 ± 0.09 This work (d)

PJ009-10 407 8.6 ± 1.2 This work (a)
346 5.9 ± 0.6 This work (b)
296 4.4 ± 0.5 This work (e)
271 3.7 ± 0.5 (1)
202 1.5 ± 0.2 This work (b)
158 0.67 ± 0.07 This work (d)

PJ036+03 671 5.6 ± 0.9 (7)
407 6.2 ± 0.7 This work (a)
334 5.0 ± 0.5 (8)
252 2.55 ± 0.3 (1)
100 0.13 ± 0.02 (9)

PJ083+11 407 10.5 ± 1.5 This work (a)
348 8.8 ± 0.9 (2)
258 5.5 ± 0.6 (10)
244 5.10 ± 0.5 (10)
145 0.9 ± 0.2 This work (f)

PJ158-14 407 9.6 ± 1.2 This work (a)
261 3.2 ± 0.3 (11)

PJ231-20 398 8.4 ± 0.9 This work (g)
337 6.8 ± 0.7 (2)
250 3.9 ± 0.4 (12)
242 3.5 ± 0.4 (12)
234 3.3 ± 0.3 (12)
227 2.9 ± 0.3 (12)
205 2.2 ± 0.2 (12)
193 1.9 ± 0.2 (12)
153 0.86 ± 0.9 (12)
140 0.72 ± 0.07 (12)
106 0.31 ± 0.04 (12)
94 0.22 ± 0.02 (12)

Notes. References – (a): ALMA projects 2019.2.00053.S and 2021.2.00064.S, (b): ALMA project 2024.1.00071.S, (c): ALMA project 2019.1.00147.S, (d): NOEMA project S24CH, (e): ALMA project 2023.1.01450.S, (f): ALMA project 2021.2.00151.S, (g): ALMA project 2022.1.00321.S, (1): Venemans et al. (2020), (2): Spilker et al. (2025), (3): Venemans et al. (2017), (4): Yang et al. (2019), (5): Yue et al. (2021), (6): Meyer et al. (2025), (7): Tripodi et al. (2024), (8): Butler et al. (2023), (9): Decarli et al. (2022), (10): Andika et al. (2020), (11): Ansarinejad et al. (2022), (12): Pensabene et al. (2021). A 10% systematic flux calibration uncertainty was added in quadrature to the nominal uncertainty when it was not already included in the reference paper. *in the fit all the fluxes have been corrected for the magnification factor reported in (5).

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