Table 5
Perturber masses creating SPHERE/PDI-ALMA substructures.
| Host ID | Min PDI | Peak PDI | Peak (mm) | Mp (min) | Mp (max) | AMES-DUSTY | BEX-HOT |
|---|---|---|---|---|---|---|---|
| (au) | (au) | (au) | (MJup) | (MJup) | (MJup) | (MJup) | |
| HD 135344B | 12 | 24 | 51 | 12.5 | >15 | 5.8 | 7.0 |
| RX J1604 | 33 | 66 | 90 | 2.2 | 9.5 | 5.1 | 6.4 |
| PDS 70 | 27 | 54 | 75 | 2.1 | 8.5 | 4.1 | 5.3 |
| HD 34282 | 44 | 89 | 138 | 4.8 | >15 | 10.0 | 11.8 |
| HD 169142 | 10 | 20 | 25 | 1.2 | 4.1 | 8.1 | 9.5 |
| LKCA 15 | 43 | 59 | 66 | <1 | 1.6 | 9.7 | 12.3 |
| HD 97048 | 127 | 188 | 189 | <1 | 1.2 | 3.9 | 5.5 |
| HD 169142 | 44 | 63 | 64 | <1 | 1.1 | 3.4 | 4.1 |
| HD 97048 | 45 | 54 | 55 | <1 | <1 | 5.6 | 7.5 |
Notes. Minimum and maximum mass of the perturbers, Mp (min) and Mp (max), respectively, calculated using Eq. (5). The derived detection limits at the perturber’s location using AMES-DUSTY and BEX-HOT tracks (best of ANDROMEDA/IRDIS and ASDI/IFS) are shown in the last two columns. References for the location of the substructures can be found in Appendix A.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.