Open Access

Table 3.

Continuum.

Frequency Synth. beam rms Flux density Size Project ID Telescope References
(GHz) (arcsec2) (mJy beam−1) (mJy) (arcsec2)
91.500 0.71 × 0.43 0.0053 0.29 ± 0.01 0.261 × 0.171 2015.1.00584.S ALMA TP, [1]
136.627 0.74 × 0.71 0.015 1.29 ± 0.03 0.345 × 0.212 2015.1.01265.S ALMA TP, [2], [3], [4]
140.995 0.79 × 0.65 0.015 1.40 ± 0.02 0.263 × 0.212 2015.1.01265.S ALMA TP, [2], [3], [4]
153.070 0.21 × 0.17 0.0091 1.63 ± 0.06 0.214 × 0.189 2018.1.00597.S ALMA This paper
263.315 0.14 × 0.11 0.016 7.73 ± 0.31 0.190 × 0.180 2018.1.00597.S ALMA This paper
265.369 1.62 × 1.3 0.056 8.81 ± 0.13 0.456 × 0.422 2019.1.01721.S ALMA This paper
284.988 0.51 × 0.39 0.073 11.05 ± 0.16 0.233 × 0.220 2013.1.00462.S ALMA TP, [3]
289.180 0.58 × 0.47 0.025 11.77 ± 0.12 0.330 × 0.246 2015.1.01265.S ALMA TP, [2], [3], [4]
344.185 0.53 × 0.43 0.051 14.63 ± 0.34 0.289 × 0.229 2015.1.01265.S ALMA TP, [2], [3], [4]
490.787 0.7 × 0.6 0.10 25.31 ± 0.19 0.318 × 0.229 2017.1.01195.S ALMA This paper, [5]
599.584 ... ... < 29.4 ... ... Herschel/SPIRE [2]
856.549 ... ... 22.0 ± 6.9 ... ... Herschel/SPIRE [2]
1199.169 ... ... 19.9 ± 6.0 ... ... Herschel/SPIRE [2]
1873.703 ... ... 13.2 ± 2.8 ... ... Herschel/PACS [2]
2997.924 ... ... 6.5 ± 1.2 ... ... Herschel/PACS [2]

Notes. All ALMA observations listed in this table are archival, and we have analysed them, even if the data-set was already been studied (see Ref. column).

References. This paper (TP); [1] Feruglio et al. (2018); [2] Shao et al. (2019); [3] Carniani et al. (2019); [4] Li et al. (2020); [5] Hashimoto et al. (2019).

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