Table 2.
Extracted fluxes for sampled GMCs.
| Source | λ [Å] | FWHM [″] | θLAS [″] | GMC 1 | GMC 2 | GMC 3 | GMC 4 | GMC 5 | GMC 6 | GMC 7 | GMC 8 | GMC 9 | GMC 10 |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| S-PLUS/uJAVA | 3563 | 1.5 | – | 0.03 | 0.03 | 0.03 | 0.04 | 0.03 | 0.04 | 0.05 | 0.06 | 0.05 | 0.04 |
| S-PLUS/J0378 | 3770 | 1.5 | – | 0.04 | 0.04 | 0.04 | 0.04 | 0.05 | 0.04 | 0.08 | 0.09 | 0.08 | 0.06 |
| S-PLUS/J0395 | 3940 | 1.5 | – | 0.05 | 0.05 | 0.05 | 0.07 | 0.06 | 0.07 | 0.11 | 0.10 | 0.11 | 0.08 |
| S-PLUS/J0410 | 4094 | 1.5 | – | 0.07 | 0.07 | 0.08 | 0.10 | 0.10 | 0.12 | 0.16 | 0.19 | 0.18 | 0.13 |
| S-PLUS/J0430 | 4292 | 1.5 | – | 0.09 | 0.09 | 0.10 | 0.13 | 0.12 | 0.14 | 0.20 | 0.24 | 0.20 | 0.18 |
| S-PLUS/gSDSS | 4751 | 1.5 | – | 0.13 | 0.15 | 0.24 | 0.31 | 0.26 | 0.30 | 0.40 | 0.44 | 0.38 | 0.31 |
| S-PLUS/J0515 | 5133 | 1.5 | – | 0.15 | 0.17 | 0.29 | 0.37 | 0.31 | 0.35 | 0.49 | 0.54 | 0.45 | 0.37 |
| HST/F555W | 5443 | 0.1 | – | – | – | – | 0.74 | 0.63 | 0.70 | 0.89 | 0.79 | – | – |
| S-PLUS/rSDSS | 6258 | 1.5 | – | 0.35 | 0.42 | 1.07 | 1.56 | 1.22 | 1.24 | 1.43 | 1.37 | 1.10 | 0.87 |
| S-PLUS/J0660 | 6614 | 1.5 | – | 0.43 | 0.56 | 1.89 | 3.27 | 2.39 | 2.16 | 2.35 | 1.94 | 1.49 | 1.13 |
| HST/F675W | 6718 | 0.1 | – | – | – | – | 2.46 | 1.96 | 1.86 | 2.05 | 1.69 | – | – |
| S-PLUS/iSDSS | 7690 | 1.5 | – | 0.65 | 0.84 | 2.56 | 3.94 | 3.08 | 2.90 | 2.80 | 2.53 | 1.91 | 1.53 |
| HST/F814W | 7996 | 0.1 | – | – | – | – | 6.28 | 4.81 | 4.15 | 3.78 | 2.98 | – | – |
| S-PLUS/J0861 | 8611 | 1.5 | – | 0.88 | 1.24 | 3.94 | 6.46 | 5.20 | 4.71 | 4.08 | 3.40 | 2.55 | 2.01 |
| S-PLUS/zSDSS | 8831 | 1.5 | – | 1.07 | 1.52 | 5.11 | 9.07 | 7.08 | 6.07 | 4.97 | 4.06 | 2.93 | 2.35 |
| HST/F850LP | 9114 | 0.13 | – | – | – | – | 12.53 | 8.93 | 6.95 | 5.48 | 3.87 | – | – |
| VLT/J | 12,650 | 0.29 | – | – | – | 22.01 | 45.75 | 31.77 | 20.08 | 9.88 | – | – | – |
| VLT/K | 21,800 | 0.24 | – | – | – | 31.16 | 93.29 | 71.15 | 39.01 | – | – | – | – |
| Spitzer/IRAC 3.6 μm | 36 000 | 1.66 | – | 2.71 | 5.72 | 28.40 | 106.38 | 109.02 | 62.01 | 23.41 | 12.60 | 6.27 | 6.30 |
| Spitzer/IRAC 4.5 μm | 45 000 | 1.72 | – | 2.43 | 4.78 | 28.08 | 150.28 | 150.45 | 69.47 | 21.64 | 10.77 | 5.20 | 5.79 |
| Spitzer/IRAC 5.8 μm | 58 000 | 1.88 | – | 7.23 | 17.75 | 121.03 | 357.56 | 464.85 | 250.73 | 89.61 | 45.28 | 22.27 | 22.98 |
| Spitzer/IRAC 8.0 μm | 80 000 | 1.98 | – | 18.98 | 52.71 | 335.32 | 1016.10 | 1095.98 | 644.08 | 243.56 | 120.51 | 60.60 | 61.62 |
| VLT/N | 118 800 | 0.4 | – | – | – | 287.88 | 3207.94 | 1273.06 | 477.52 | 121.49 | – | – | – |
| VLT/Q | 187 200 | 0.74 | – | – | – | 1178.25 | 18901.04 | 9984.58 | 3340.52 | 654.91 | 355.37 | – | – |
| ALMA/B7 | 9 252 854 | 1.6 | 15 | 11.48 | 9.63 | 188.92 | 289.28 | 343.56 | 255.51 | 51.86 | 18.37 | 18.35 | 17.51 |
| ALMA/B6 | 12 337 138 | 1.6 | 15 | 2.58 | 3.28 | 68.74 | 122.77 | 165.38 | 103.49 | 17.11 | 5.82 | 5.17 | 6.45 |
| ALMA/B5 | 16 031 682 | 1.6 | 15 | 2.85 | 1.91 | 35.92 | 72.02 | 110.39 | 58.05 | 8.34 | 3.07 | 2.86 | 2.64 |
| ALMA/B4 | 20 818 921 | 1.6 | 15 | 1.29 | 1.57 | 24.13 | 56.96 | 101.44 | 40.57 | 5.76 | 2.37 | 1.69 | 2.50 |
| ALMA/B3 | 29 979 246 | 1.6 | 15 | – | – | 18.41 | 50.46 | 102.15 | 33.61 | 3.60 | – | – | 1.27 |
| EVLA band Ka (DnC) | 91,330,642 | 1.76 × 1.39 | 44 | – | – | 21.80 | 59.07 | 141.84 | 40.53 | 4.91 | – | – | 1.54 |
| VLA band K (B) | 127 245 834 | 0.47 × 0.26 | 7.9 | – | – | – | – | 135.60 | – | – | – | – | – |
| VLA band Ku (B) | 200 665 639 | 0.67 × 0.40 | 12 | – | – | 30.67 | 71.92 | 181.58 | 50.21 | – | – | – | – |
| EVLA band X (A) | 299 773 911 | 0.46 × 0.19 | 5.3 | – | – | – | 98.03 | 264.56 | 81.33 | – | – | – | – |
| VLA band C (A) | 616 844 217 | 0.69 × 0.39 | 8.9 | – | – | 41.34 | 104.45 | 318.02 | 70.16 | 9.08 | – | – | – |
| VLA band L (A) | 2 012 164 964 | 2.13 × 1.25 | 36 | 6.57 | 12.38 | 89.09 | 175.32 | 274.92 | 160.83 | 36.35 | 16.68 | 15.20 | 5.69 |
Notes. Column 5 through the last column display the extracted fluxes [mJy] for each sampled GMC within a 3″ aperture diameter. A dash – indicates the lack of (enough) data filling the aperture. Uncertainties were assumed to be of the order of 10% for all the sample except for ALMA data, where we assume 15%. Additionally, observational parameters, namely, wavelength, FWHM of the beam/psf, and largest angular scales in the case of interferometric observations are indicated in columns 2, 3, and 4, respectively, while the first column specifies the source (facility or survey) and filter, plus the array configuration mode provided parenthetically for the (E)VLA observations. The largest angular scale, θLAS, is pertinent for interferometric observations only, namely: ALMA (Martín et al. 2021), EVLA (https://science.nrao.edu/facilities/vla/docs/manuals/oss2012B/performance/referencemanual-all-pages), and VLA (https://science.nrao.edu/facilities/vla/docs/manuals/oss/performance/resolution).
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