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Table 3
Comparison of predicted and observed planetary masses in PCEBs with more than one planet.
| System | α L | m th,1 | m o,1 | m th,2 | m o,2 |
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| HW Vir | 12.5 | 6.8 | 30 − 120 | 0.6 | 14.3 |
| NY Vir | 9.5 | 6.2 | 2.5 | 2.4 | 2.3 |
| NN Ser | 12.5 | 6.6 | 7.0 | 1.9 | 1.7 |
| QS Vir | 6.0 | 13.5 | 56.59 | 9.0 | 9.01 |
| UZ For | 13.5 | 8.6 | 7.7 | 1.4 | 6.3 |
Notes. Here, αL is calibrated based on the largest observed orbit, mth,1 and mth,2 are the expected planetary masses at the locations of the observed orbits, and mo,1, mo,2 are the observed masses of the planets.
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