Open Access
Table B.1.
Best-fitting parameters of the companions derived using Bagpipes and Dense Basis.
| ID | log M★/M⊙ | log SFR [M⊙/yr] | Av [mag] | log M★/M⊙ | log SFR [M⊙/yr] | Av [mag] |
| Bagpipes | Dense Basis | |||||
| C1 | 8.69![]() |
0.700.670.74 | 0.61![]() |
9.04![]() |
0.70![]() |
0.43![]() |
| C2 | 8.00![]() |
![]() |
0.14![]() |
8.10![]() |
![]() |
0.23![]() |
| C3 | 8.45![]() |
![]() |
0.23![]() |
8.50![]() |
![]() |
0.22![]() |
Notes. We include the 16th and 84th percentiles. The star formation rates correspond to SFR100.
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