Table 1
Final properties of the RM and its variants at 15 Gyr.
| Model | M ∗ | M esc | M BH | MBH/M∗ | log ⟨ NH ⟩ |
|
|
ΔtCT | Δtobs | Δtunobs | ||
|
|
||||||||||||
| RM | 93.22 | 6.56 | 0.256 | 2.75 × 10-3 | 20.05 | 10.42 | 7.94 | 2.17 | 9.57 | 3.26 | ||
| RM1 | 92.47 | 6.62 | 0.945 | 1.02 × 10-2 | 20.04 | 10.37 | 7.91 | 2.13 | 9.56 | 3.31 | ||
| RM2 | 42.65 | 7.21 | 0.214 | 5.01 × 10-3 | 19.63 | 8.42 | 5.78 | 0.00 | 10.33 | 4.67 | ||
| RM3 | 192.97 | 6.69 | 0.321 | 1.67 × 10-3 | 20.46 | 12.04 | 9.69 | 4.92 | 8.17 | 1.91 | ||
| RM4 | 90.59 | 5.55 | 0.288 | 3.18 × 10-3 | 22.81 | 14.20 | 10.47 | 0.00 | 14.99 | 0.01 | ||
Notes. All masses are in 109 M⊙ units. MBH is the final black hole mass; M∗ is the final stellar mass; Mesc is the total escaped gas mass. The average column density is in cm-2. ΔtCT, Δtobs, and Δtunobs represent the durations (in Gyr) of the Compton-thick phase, of the obscured phase, and the unobscured phase, respectively. Finally, and are the durations (in Gyr) measured assuming threshold temperatures of 105 K and 5 × 104 K, respectively.
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