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Table 3
Reference systems for our simulated ALMA observations.
| Run | Reference | λ ref | d | Host star | Age | R dust | Fdisk at λref | M disk | Ref. |
| [ μm] | [pc] | [Myr] | [AU] | [mJy] | [M⊙] | ||||
|
|
|||||||||
| Ib | ϵ Eri | 24 | 3.2 | K2 V | 850 | 3.0 | 330.0 | 5.7 × 10-11 | 1 |
| Ic | HD 105 | 850 | 40.0 | G0 V | 30 | 45–120 | 10.7 | 1.2 × 10-7 | 2 |
| IIc | HD 107146 | 350 | 29.5 | G2 V | 130 | 50–250 | 319.0 | 7.3 × 10-7 | 3, 4 |
| IIIa | HD 107146 | 350 | 29.5 | G2 V | 130 | 50–250 | 319.0 | 3.7 × 10-7 | 3, 4 |
| IIId | HD 107146 | 350 | 29.5 | G2 V | 130 | 50–250 | 319.0 | 5.5 × 10-7 | 3, 4 |
References. (1) Backman et al. (2009); (2) Nilsson et al. (2010); (3) Corder et al. (2009); (4) Ertel et al. (2011).
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