Table 1.

Simulation results.

IDηfboundfboundfboundfboundfbound
0.2Tr0.4Tr0.6Tr0.8TrTr
(1)(2)(3)(4)(5)(6)(7)
S00.00.9820.9090.1200.1110.110
S10.10.9820.9080.2620.2440.230
S20.20.9820.9050.3670.3470.323
S30.30.9810.9010.4290.4090.378
S40.40.9810.8940.4790.4540.419
S50.50.9800.8870.5220.4890.453
S60.60.9790.8770.5590.5200.484
S70.70.9770.8670.5940.5500.514
S80.80.9750.8580.6310.5800.543
S90.90.9690.8490.6720.6120.573
S101.00.9420.8370.7320.6640.613
IDηfboundfboundfboundfboundfbound
0.2Tr0.4Tr0.6Tr0.8TrTr
(1)(2)(3)(4)(5)(6)(7)
S00.00.9820.9090.1200.1110.110
S10.10.9820.9080.2620.2440.230
S20.20.9820.9050.3670.3470.323
S30.30.9810.9010.4290.4090.378
S40.40.9810.8940.4790.4540.419
S50.50.9800.8870.5220.4890.453
S60.60.9790.8770.5590.5200.484
S70.70.9770.8670.5940.5500.514
S80.80.9750.8580.6310.5800.543
S90.90.9690.8490.6720.6120.573
S101.00.9420.8370.7320.6640.613

Note. The bound fractions at five different epochs, t/Tr = 0.2, 0.4, ..., 1.0 (Columns 3–7), inferred from our idealized simulations of subhaloes orbiting in the fixed potential of an NFW host. Each simulation has Mh/Ms = 1000, ch = 5, cs = 10 and xc = 1.0, and only differ in their value for the orbital circularity, η (Column 2). In each simulation, the subhalo, which is simulated with N = 107 particles, starts out at its own apo-centre (cf. Fig. 2).

Table 1.

Simulation results.

IDηfboundfboundfboundfboundfbound
0.2Tr0.4Tr0.6Tr0.8TrTr
(1)(2)(3)(4)(5)(6)(7)
S00.00.9820.9090.1200.1110.110
S10.10.9820.9080.2620.2440.230
S20.20.9820.9050.3670.3470.323
S30.30.9810.9010.4290.4090.378
S40.40.9810.8940.4790.4540.419
S50.50.9800.8870.5220.4890.453
S60.60.9790.8770.5590.5200.484
S70.70.9770.8670.5940.5500.514
S80.80.9750.8580.6310.5800.543
S90.90.9690.8490.6720.6120.573
S101.00.9420.8370.7320.6640.613
IDηfboundfboundfboundfboundfbound
0.2Tr0.4Tr0.6Tr0.8TrTr
(1)(2)(3)(4)(5)(6)(7)
S00.00.9820.9090.1200.1110.110
S10.10.9820.9080.2620.2440.230
S20.20.9820.9050.3670.3470.323
S30.30.9810.9010.4290.4090.378
S40.40.9810.8940.4790.4540.419
S50.50.9800.8870.5220.4890.453
S60.60.9790.8770.5590.5200.484
S70.70.9770.8670.5940.5500.514
S80.80.9750.8580.6310.5800.543
S90.90.9690.8490.6720.6120.573
S101.00.9420.8370.7320.6640.613

Note. The bound fractions at five different epochs, t/Tr = 0.2, 0.4, ..., 1.0 (Columns 3–7), inferred from our idealized simulations of subhaloes orbiting in the fixed potential of an NFW host. Each simulation has Mh/Ms = 1000, ch = 5, cs = 10 and xc = 1.0, and only differ in their value for the orbital circularity, η (Column 2). In each simulation, the subhalo, which is simulated with N = 107 particles, starts out at its own apo-centre (cf. Fig. 2).

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