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Table 3

Approximate upper mass limits of a putative perturber in various orbital resonances for each system.

MMR WASP-18A WASP-19 WASP-77A
(P2P1) [M] [M] [M]
1:4 4.0
1:3 2.5 70.0(a)
2:5 1.0
1:2 9.0(b) 0.26 1.8
4:7 1.5
3:5 8.0
2:3 5.5(b)
11:7 3.0
5:3 2.8 6.0
7:4 5.5
2:1 11.0(b) 0.65 3.0
7:3 6.5
5:2 7.5 3.0 105.0(c)
3:1 4.0 1.0 50.0(d)
17:5 350.0(e)
4:1 7.5 95.0(f) 35.0(g)

Notes. (a) Upper mass limit from RV: 13.4 M. (b) Very close to the gene- ral instability area. (c)Upper mass limit from RV: 26.4 M. (d) Upper mass limit from RV: 28.0 M. (e) Upper mass limit from RV: 82.8 M. (f) Upper mass limit from RV: 40.8 M. (g) Upper mass limit from RV: 30.8 M.

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