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Table A.16
Masses from 870 μm dust emission and virial masses for subsample S1.
| Source | M | 68%int. | M vir | 68%int. | Group | ||
| (103 × M⊙) | (103 × M⊙) | (103 × M⊙) | (103 × M⊙) | ||||
|
|
|||||||
| AGAL008.684-00.367 | 17.40 | 7.46 − 24.78 | 3.62 | 2.77 − 4.52 | D8 | ||
| AGAL008.706-00.414 | 14.97 | 5.83 − 20.39 | 1.50 | 0.96 − 1.96 | D24 | ||
| AGAL010.444-00.017 | 10.09 | 3.51 − 13.94 | 1.80 | 1.19 − 2.30 | D24 | ||
| AGAL010.472+00.027 | 19.99 | 6.07 − 27.62 | 8.35 | 6.02 − 10.36 | IRB | ||
| AGAL010.624-00.384 | 1.06 | 0.37 − 1.52 | 1.78 | 1.32 − 2.21 | IRB | ||
| AGAL012.804-00.199 | 2.21 | 1.29 − 3.02 | 2.44 | 2.19 − 2.67 | IRB | ||
| AGAL013.178+00.059 | 18.76 | 5.91 − 26.07 | 3.20 | 2.32 − 4.07 | D8 | ||
| AGAL013.658-00.599 | 0.99 | 0.37 − 1.41 | 0.73 | 0.51 − 0.91 | RMS | ||
| AGAL014.114-00.574 | 0.53 | 0.20 − 0.75 | 0.46 | 0.35 − 0.57 | D8 | ||
| AGAL014.194-00.194 | 1.93 | 0.73 − 2.63 | 1.20 | 0.12 − 1.75 | D8 | ||
| AGAL014.492-00.139 | 2.65 | 1.07 − 3.71 | 1.74 | 1.10 − 2.31 | D24 | ||
| AGAL014.632-00.577 | 0.32 | 0.13 − 0.46 | 0.52 | 0.39 − 0.65 | D8 | ||
| AGAL015.029-00.669-1 | 0.57 | 0.25 − 0.74 | 1.04 | 0.94 − 1.14 | IRB | ||
| AGAL018.606-00.074 | 7.31 | 2.83 − 9.87 | 1.95 | 1.03 − 2.56 | D24 | ||
| AGAL018.734-00.226 | 16.75 | 7.16 − 23.56 | 6.52 | 4.30 − 8.53 | D8 | ||
| AGAL018.888-00.474 | 2.08 | 0.82 − 2.94 | 2.56 | 1.98 − 3.21 | D8 | ||
| AGAL019.882-00.534 | 0.44 | 0.10 − 0.62 | 0.78 | 0.57 − 0.95 | RMS | ||
| AGAL022.376+00.447-1 | 1.32 | 0.52 − 1.84 | 0.13 | 0.08 − 0.17 | D24 | ||
| AGAL023.206-00.377 | 2.58 | 0.99 − 3.56 | 1.48 | 1.11 − 1.84 | D8 | ||
| AGAL024.629+00.172-1 | 2.26 | 0.87 − 3.04 | 1.86 | 1.15 − 2.47 | D24 | ||
| AGAL028.564-00.236 | 7.22 | 3.07 − 10.29 | 3.10 | 1.80 − 4.22 | D24 | ||
| AGAL028.861+00.066-1 | 1.41 | 0.48 − 2.00 | 1.44 | 1.08 − 1.77 | RMS | ||
| AGAL030.848-00.081-1 | 2.39 | 0.88 − 3.34 | 1.75 | 1.09 − 2.20 | D24 | ||
| AGAL030.893+00.139-2 | 2.44 | 0.99 − 3.41 | 2.01 | 0.96 − 2.67 | D24 | ||
| AGAL031.412+00.307 | 4.41 | 2.21 − 5.95 | 2.69 | 2.27 − 3.15 | IRB | ||
| AGAL034.258+00.154 | 1.40 | 0.36 − 2.02 | 1.33 | 0.96 − 1.75 | IRB | ||
| AGAL034.401+00.226 | 0.42 | 0.27 − 0.53 | 0.90 | 0.81 − 0.99 | RMS | ||
| AGAL034.411+00.234 | 0.28 | 0.18 − 0.37 | 0.47 | 0.39 − 0.55 | D8 | ||
| AGAL034.821+00.351 | 1.23 | 0.45 − 1.70 | 0.82 | 0.61 − 1.01 | RMS | ||
| AGAL035.197-00.742 | 0.75 | 0.45 − 0.98 | 0.83 | 0.73 − 0.93 | RMS | ||
| AGAL037.554+00.201 | 2.24 | 0.81 − 3.15 | 1.81 | 1.34 − 2.23 | RMS | ||
| AGAL043.166+00.011-1 | 17.09 | 11.08 − 22.12 | 26.31 | 22.36 − 29.62 | IRB | ||
| AGAL049.489-00.389 | 8.93 | 4.93 − 11.72 | 5.29 | 4.75 − 5.68 | IRB | ||
| AGAL053.141+00.069 | 0.14 | 0.06 − 0.20 | 0.41 | 0.30 − 0.51 | RMS | ||
| AGAL059.782+00.066 | 0.27 | 0.18 − 0.35 | 0.35 | 0.32 − 0.39 | RMS | ||
Notes. The columns show the mass derived from the dust continuum emission and the virial mass, with their respective uncertainties. The last column indicates the group of the source.
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