Table 2
Observational data summary of the 12 m array continuum images of ALMA-IMF protoclusters.
1.3 mm (Band 6) | 3 mm (Band 3) | ||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|
Protocluster | Imaged FOV(1) | Resolution (2) | σ(cleanest)(3) | σ(bsens)(3) | ![]() |
Imaged FOV (1) | Resolution (2) | σ(cleanest)(3) | σ(bsens)(3) | ![]() |
|
cloud name | [″ × ″] | [″ × ″] | [mJy beam−1] | [″] | [″ × ″] | [″ × ″] | [mJy beam−1] | [″] | |||
W51-E | 100 × 90 | 0.35 × 0.27 | 0.17 | 0.16 | 5.0 | 150 × 160 | 0.29 × 0.26 | 0.055 | 0.035 | 6.3 | |
W43-MM1 | 117 × 53 | 0.50 × 0.35 | 0.19 | 0.18 | 4.6 | 190 × 150 | 0.56 × 0.33 | 0.051 | 0.038 | 4.8 | |
G333.60 | 143 × 143 | 0.56 × 0.51 | 0.11 | 0.12 | 5.8 | 190 × 180 | 0.46 × 0.44 | 0.070 | 0.047 | 10 | |
W51-IRS2 | 92 × 98 | 0.50 × 0.44 | 0.097 | 0.076 | 6.1 | 160 × 150 | 0.28 × 0.27 | 0.061 | 0.061 | 9.6 | |
G338.93 | 86 × 92 | 0.56 × 0.51 | 0.17 | 0.16 | 5.5 | 152 × 160 | 0.40 × 0.38 | 0.068 | 0.044 | 11 | |
G010.62 | 98 × 90 | 0.53 × 0.41 | 0.083 | 0.082 | 5.2 | 150 × 160 | 0.39 × 0.32 | 0.051 | 0.051 | 9.4 | |
W43-MM2 | 90 × 98 | 0.52 × 0.41 | 0.075 | 0.063 | 5.5 | 190 × 150 | 0.30 × 0.24 | 0.037 | 0.024 | 8.1 | |
G008.67 | 132 × 87 | 0.72 × 0.59 | 0.37 | 0.20 | 5.9 | 190 × 125 | 0.51 × 0.40 | 0.094 | 0.080 | 10 | |
G012.80 | 132 × 132 | 1.09 × 0.70 | 0.65 | 0.74 | 6.6 | 190 × 180 | 1.48 × 1.26 | 0.21 | 0.24 | 9.9 | |
G327.29 | 105 × 109 | 0.69 × 0.62 | 0.36 | 0.32 | 5.5 | 160 × 152 | 0.43 × 0.37 | 0.13 | 0.075 | 10 | |
W43-MM3 | 100 × 90 | 0.51 × 0.43 | 0.061 | 0.063 | 5.7 | 190 × 150 | 0.41 × 0.29 | 0.031 | 0.028 | 8.2 | |
G351.77 | 132 × 132 | 0.89 × 0.67 | 0.42 | 0.31 | 6.2 | 190 ×180 | 1.52 × 1.30 | 0.26 | 0.12 | 15 | |
G353.41 | 131 × 131 | 0.93 × 0.66 | 0.42 | 0.40 | 6.2 | 190 × 180 | 1.46 × 1.27 | 0.18 | 0.17 | 10 | |
G337.92 | 92 × 86 | 0.61 × 0.48 | 0.22 | 0.23 | 5.6 | 160 × 152 | 0.45 × 0.38 | 0.070 | 0.051 | 11 | |
G328.25 | 120 × 120 | 0.62 × 0.47 | 0.37 | 0.29 | 4.9 | 160 × 180 | 0.62 × 0.44 | 0.087 | 0.076 | 7.5 |
Notes. (1)Field of view (FOV) corresponding to the combined primary beam of the 1.3 mm and 3 mm mosaics, down to 15% of the peak sensitivity. (2)Angular resolution resulting from a tclean process with the Briggs robust parameter robust=0. (3)Noise level measured in the bsens and cleanest 12 m array images at 1.3 mm and 3 mm. (4)The maximum recoverable scale of the 12 m array, often called the largest angular scale (LAS), is estimated for each 1.3 m and 3 mm images as the 10th percentile of the baseline lengths of 12 m array data (see Figs. 5–7 of Ginsburg et al. 2022).
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