ID . | η . | fbound . | fbound . | fbound . | fbound . | fbound . |
---|---|---|---|---|---|---|
. | . | 0.2Tr . | 0.4Tr . | 0.6Tr . | 0.8Tr . | Tr . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
S0 | 0.0 | 0.982 | 0.909 | 0.120 | 0.111 | 0.110 |
S1 | 0.1 | 0.982 | 0.908 | 0.262 | 0.244 | 0.230 |
S2 | 0.2 | 0.982 | 0.905 | 0.367 | 0.347 | 0.323 |
S3 | 0.3 | 0.981 | 0.901 | 0.429 | 0.409 | 0.378 |
S4 | 0.4 | 0.981 | 0.894 | 0.479 | 0.454 | 0.419 |
S5 | 0.5 | 0.980 | 0.887 | 0.522 | 0.489 | 0.453 |
S6 | 0.6 | 0.979 | 0.877 | 0.559 | 0.520 | 0.484 |
S7 | 0.7 | 0.977 | 0.867 | 0.594 | 0.550 | 0.514 |
S8 | 0.8 | 0.975 | 0.858 | 0.631 | 0.580 | 0.543 |
S9 | 0.9 | 0.969 | 0.849 | 0.672 | 0.612 | 0.573 |
S10 | 1.0 | 0.942 | 0.837 | 0.732 | 0.664 | 0.613 |
ID . | η . | fbound . | fbound . | fbound . | fbound . | fbound . |
---|---|---|---|---|---|---|
. | . | 0.2Tr . | 0.4Tr . | 0.6Tr . | 0.8Tr . | Tr . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
S0 | 0.0 | 0.982 | 0.909 | 0.120 | 0.111 | 0.110 |
S1 | 0.1 | 0.982 | 0.908 | 0.262 | 0.244 | 0.230 |
S2 | 0.2 | 0.982 | 0.905 | 0.367 | 0.347 | 0.323 |
S3 | 0.3 | 0.981 | 0.901 | 0.429 | 0.409 | 0.378 |
S4 | 0.4 | 0.981 | 0.894 | 0.479 | 0.454 | 0.419 |
S5 | 0.5 | 0.980 | 0.887 | 0.522 | 0.489 | 0.453 |
S6 | 0.6 | 0.979 | 0.877 | 0.559 | 0.520 | 0.484 |
S7 | 0.7 | 0.977 | 0.867 | 0.594 | 0.550 | 0.514 |
S8 | 0.8 | 0.975 | 0.858 | 0.631 | 0.580 | 0.543 |
S9 | 0.9 | 0.969 | 0.849 | 0.672 | 0.612 | 0.573 |
S10 | 1.0 | 0.942 | 0.837 | 0.732 | 0.664 | 0.613 |
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).
ID . | η . | fbound . | fbound . | fbound . | fbound . | fbound . |
---|---|---|---|---|---|---|
. | . | 0.2Tr . | 0.4Tr . | 0.6Tr . | 0.8Tr . | Tr . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
S0 | 0.0 | 0.982 | 0.909 | 0.120 | 0.111 | 0.110 |
S1 | 0.1 | 0.982 | 0.908 | 0.262 | 0.244 | 0.230 |
S2 | 0.2 | 0.982 | 0.905 | 0.367 | 0.347 | 0.323 |
S3 | 0.3 | 0.981 | 0.901 | 0.429 | 0.409 | 0.378 |
S4 | 0.4 | 0.981 | 0.894 | 0.479 | 0.454 | 0.419 |
S5 | 0.5 | 0.980 | 0.887 | 0.522 | 0.489 | 0.453 |
S6 | 0.6 | 0.979 | 0.877 | 0.559 | 0.520 | 0.484 |
S7 | 0.7 | 0.977 | 0.867 | 0.594 | 0.550 | 0.514 |
S8 | 0.8 | 0.975 | 0.858 | 0.631 | 0.580 | 0.543 |
S9 | 0.9 | 0.969 | 0.849 | 0.672 | 0.612 | 0.573 |
S10 | 1.0 | 0.942 | 0.837 | 0.732 | 0.664 | 0.613 |
ID . | η . | fbound . | fbound . | fbound . | fbound . | fbound . |
---|---|---|---|---|---|---|
. | . | 0.2Tr . | 0.4Tr . | 0.6Tr . | 0.8Tr . | Tr . |
(1) . | (2) . | (3) . | (4) . | (5) . | (6) . | (7) . |
S0 | 0.0 | 0.982 | 0.909 | 0.120 | 0.111 | 0.110 |
S1 | 0.1 | 0.982 | 0.908 | 0.262 | 0.244 | 0.230 |
S2 | 0.2 | 0.982 | 0.905 | 0.367 | 0.347 | 0.323 |
S3 | 0.3 | 0.981 | 0.901 | 0.429 | 0.409 | 0.378 |
S4 | 0.4 | 0.981 | 0.894 | 0.479 | 0.454 | 0.419 |
S5 | 0.5 | 0.980 | 0.887 | 0.522 | 0.489 | 0.453 |
S6 | 0.6 | 0.979 | 0.877 | 0.559 | 0.520 | 0.484 |
S7 | 0.7 | 0.977 | 0.867 | 0.594 | 0.550 | 0.514 |
S8 | 0.8 | 0.975 | 0.858 | 0.631 | 0.580 | 0.543 |
S9 | 0.9 | 0.969 | 0.849 | 0.672 | 0.612 | 0.573 |
S10 | 1.0 | 0.942 | 0.837 | 0.732 | 0.664 | 0.613 |
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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