Table 4.
Open in new tab

Summary statistics of BH masses in Pop III BBH mergers for the 18 models listed in Table 2. The second, third, and last columns show the average chirp mass |$m_{\rm c}$|⁠, primary mass |$m_{1}$|⁠, and mass ratio q for BBH mergers in galaxy fields/NSCs.

Model|$\bar{m}_{\rm c}^{\rm field/NSC}$||$\bar{m}_{\rm 1}^{\rm field/NSC}$||$\bar{q}^{\rm field/NSC}$|
|$\rm [M_{\odot }]$||$\rm [M_{\odot }]$|
LOG1_obs23.4/97.231.3/1600.75/0.64
TOP1_obs25.3/16933.8/2820.76/0.58
KRO1_obs20.4/38.428.1/56.70.71/0.71
LOG5_obs25.8/13137/2420.69/0.55
TOP5_obs27.9/18541.7/3450.68/0.48
KRO5_obs24.4/58.334.6/94.30.7/0.68
LOG1_full23.4/94.231.3/1540.75/0.64
TOP1_full25.2/16533.5/2760.77/0.58
KRO1_full20.4/37.528/55.40.71/0.7
LOG5_full25.6/12936.5/2380.69/0.55
TOP5_full26.2/18238.1/3410.68/0.48
KRO5_full24.3/57.334.4/92.20.7/0.69
LOG1_low23.4/10731.3/1740.75/0.64
TOP1_low25.2/18033.6/2950.76/0.58
KRO1_low20.4/40.528.1/59.90.71/0.71
LOG5_low25.6/14336.6/2610.69/0.54
TOP5_low26.3/19338.3/3570.68/0.48
KRO5_low24.2/63.434.4/1040.7/0.68
Model|$\bar{m}_{\rm c}^{\rm field/NSC}$||$\bar{m}_{\rm 1}^{\rm field/NSC}$||$\bar{q}^{\rm field/NSC}$|
|$\rm [M_{\odot }]$||$\rm [M_{\odot }]$|
LOG1_obs23.4/97.231.3/1600.75/0.64
TOP1_obs25.3/16933.8/2820.76/0.58
KRO1_obs20.4/38.428.1/56.70.71/0.71
LOG5_obs25.8/13137/2420.69/0.55
TOP5_obs27.9/18541.7/3450.68/0.48
KRO5_obs24.4/58.334.6/94.30.7/0.68
LOG1_full23.4/94.231.3/1540.75/0.64
TOP1_full25.2/16533.5/2760.77/0.58
KRO1_full20.4/37.528/55.40.71/0.7
LOG5_full25.6/12936.5/2380.69/0.55
TOP5_full26.2/18238.1/3410.68/0.48
KRO5_full24.3/57.334.4/92.20.7/0.69
LOG1_low23.4/10731.3/1740.75/0.64
TOP1_low25.2/18033.6/2950.76/0.58
KRO1_low20.4/40.528.1/59.90.71/0.71
LOG5_low25.6/14336.6/2610.69/0.54
TOP5_low26.3/19338.3/3570.68/0.48
KRO5_low24.2/63.434.4/1040.7/0.68
Table 4.
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Summary statistics of BH masses in Pop III BBH mergers for the 18 models listed in Table 2. The second, third, and last columns show the average chirp mass |$m_{\rm c}$|⁠, primary mass |$m_{1}$|⁠, and mass ratio q for BBH mergers in galaxy fields/NSCs.

Model|$\bar{m}_{\rm c}^{\rm field/NSC}$||$\bar{m}_{\rm 1}^{\rm field/NSC}$||$\bar{q}^{\rm field/NSC}$|
|$\rm [M_{\odot }]$||$\rm [M_{\odot }]$|
LOG1_obs23.4/97.231.3/1600.75/0.64
TOP1_obs25.3/16933.8/2820.76/0.58
KRO1_obs20.4/38.428.1/56.70.71/0.71
LOG5_obs25.8/13137/2420.69/0.55
TOP5_obs27.9/18541.7/3450.68/0.48
KRO5_obs24.4/58.334.6/94.30.7/0.68
LOG1_full23.4/94.231.3/1540.75/0.64
TOP1_full25.2/16533.5/2760.77/0.58
KRO1_full20.4/37.528/55.40.71/0.7
LOG5_full25.6/12936.5/2380.69/0.55
TOP5_full26.2/18238.1/3410.68/0.48
KRO5_full24.3/57.334.4/92.20.7/0.69
LOG1_low23.4/10731.3/1740.75/0.64
TOP1_low25.2/18033.6/2950.76/0.58
KRO1_low20.4/40.528.1/59.90.71/0.71
LOG5_low25.6/14336.6/2610.69/0.54
TOP5_low26.3/19338.3/3570.68/0.48
KRO5_low24.2/63.434.4/1040.7/0.68
Model|$\bar{m}_{\rm c}^{\rm field/NSC}$||$\bar{m}_{\rm 1}^{\rm field/NSC}$||$\bar{q}^{\rm field/NSC}$|
|$\rm [M_{\odot }]$||$\rm [M_{\odot }]$|
LOG1_obs23.4/97.231.3/1600.75/0.64
TOP1_obs25.3/16933.8/2820.76/0.58
KRO1_obs20.4/38.428.1/56.70.71/0.71
LOG5_obs25.8/13137/2420.69/0.55
TOP5_obs27.9/18541.7/3450.68/0.48
KRO5_obs24.4/58.334.6/94.30.7/0.68
LOG1_full23.4/94.231.3/1540.75/0.64
TOP1_full25.2/16533.5/2760.77/0.58
KRO1_full20.4/37.528/55.40.71/0.7
LOG5_full25.6/12936.5/2380.69/0.55
TOP5_full26.2/18238.1/3410.68/0.48
KRO5_full24.3/57.334.4/92.20.7/0.69
LOG1_low23.4/10731.3/1740.75/0.64
TOP1_low25.2/18033.6/2950.76/0.58
KRO1_low20.4/40.528.1/59.90.71/0.71
LOG5_low25.6/14336.6/2610.69/0.54
TOP5_low26.3/19338.3/3570.68/0.48
KRO5_low24.2/63.434.4/1040.7/0.68
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