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Table 3

Fraction of the compact binaries with eccentricity greater than 10-2.

NS-NS

30 Hz 3 Hz 0.3 Hz

AZK 0. 60% (51) 1. 32% (112) 11. 13% (945)
BZK 1. 27% (36) 2. 33% (66) 6. 52% (185)
AZk 0. 16% (27) 0. 38% (64) 10. 37% (1732)
BZk 0. 30% (15) 0. 75% (37) 2. 22% (110)
AzK 0. 29% (25) 0. 96% (83) 21. 74% (1880)
BzK 1. 87% (13) 4. 02% (28) 9. 33% (65)
Azk 0. 26% (37) 0. 57% (81) 26. 91% (3799)
Bzk 1. 74% (21) 3. 31% (40) 7. 79% (94)
BH-NS

30 Hz 3 Hz 0.3 Hz

AZK 0. 29% (2) 0. 73% (5) 3. 05% (21)
AZk 0. 15% (2) 0. 54% (7) 0. 61% (8)
AzK 0. 56% (14) 0. 96% (24) 3. 96% (99)
BzK 0. 68% (10) 1. 23% (18) 3. 63% (53)
Azk 0. 35% (15) 0. 78% (34) 2. 81% (122)
Bzk 0. 33% (8) 0. 91% (22) 1. 53% (37)
BH-BH

30 Hz 3 Hz 0.3 Hz

AZK 0. 31% (1) 0. 62% (2) 1. 87% (6)
AzK 0. 02% (3) 0. 02% (4) 0. 13% (23)
BzK 0. 15% (2) 0. 15% (2) 0. 46% (6)
Azk 0. 00% (1) 0. 01% (2) 0. 03% (6)

Notes. Top table corresponds to double neutron stars (NS-NS), middle to the mixed systems (BH-NS), and the bottom to the binary black holes (BH-BH). We present the fraction of binaries at the moment of entering different frequency bands (30 Hz, 3 Hz, and 0.3 Hz). In brackets, we include the number of these systems in the simulation N. We only listed results for models that are non-zero. The number of digits shown is for formatting only, and the relative sampling error is N − 1/2.

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