Table B.1.
Observable properties of GW host galaxies.
Event | Redshift | Distance between galaxy | ℳc | Lx | LCII | LFIR | Apparent | Mab | S/N | Angular Resolution |
---|---|---|---|---|---|---|---|---|---|---|
Number | and BH (physical kpc) | (M/M⊙) | (ergs/s) | (L/L⊙) | (L/L⊙) | Magnitude | Ω (Deg2) | |||
1 | 6 | 0.48 | 1.9 × 106 | 1.4 × 1042 | 2.1 × 108 | 3 × 1012 | 28.01 | -20.85 | 24.12 | 859.33 |
2 | 6 | 0.08 | 2.4 × 107 | 6.2 × 1044 | 3.9 × 109 | 4.4 × 1013 | 23.26 | -25.60 | Not Detectable | Not Applicable |
3 | 6.09 | 0.51 | 6.2 × 105 | 4.1 × 1039 | 3.5 × 104 | 1.7 × 1010 | 34.46 | -14.44 | 164.27 | 18.53 |
4 | 6.12 | 0.59 | 1.9 × 107 | 2.6 × 1044 | 3.2 × 109 | 3.8 × 1013 | 24.34 | -24.57 | Not Detectable | Not Applicable |
5 | 6.13 | 3.57 | 1.2 × 106 | 2.8 × 1042 | 3.7 × 108 | 1.2 × 1013 | 27.48 | -21.42 | 89.62 | 62.25 |
6 | 6.17 | 4.36 | 9.1 × 105 | 9.5 × 1043 | 2.5 × 109 | 3.3 × 1013 | 25.25 | -23.69 | 129.01 | 30.04 |
7 | 6.19 | 0.89 | 1.8 × 106 | 7.1 × 1041 | 1.5 × 108 | 3.8 × 1012 | 28.27 | -20.68 | 32.90 | 461.85 |
8 | 6.22 | 1.55 | 1.6 × 106 | 1.5 × 1042 | 1.4 × 108 | 2.3 × 1012 | 28.4 | -20.55 | 45.29 | 243.81 |
9 | 6.22 | 1.84 | 8.9 × 105 | 2.8 × 1042 | 3.6 × 108 | 1.2 × 1013 | 27.56 | -21.38 | 131.39 | 28.96 |
10 | 6.29 | 0.82 | 1.7 × 106 | 7 × 1041 | 1.4 × 108 | 3.8 × 1012 | 28.35 | -20.64 | 40.86 | 299.42 |
11 | 6.29 | 0.22 | 1.6 × 107 | 1.1 × 1044 | 1.6 × 109 | 2.6 × 1013 | 25.42 | -23.56 | Not Detectable | Not Applicable |
12 | 6.3 | 0.34 | 1.3 × 106 | 1.3 × 1042 | 1 × 108 | 2.4 × 1012 | 28.64 | -20.35 | 69.82 | 102.57 |
13 | 6.31 | 1.08 | 6.4 × 105 | 5 × 1039 | 1.2 × 105 | 3 × 1010 | 33.31 | -15.67 | 156.91 | 20.31 |
14 | 6.36 | 0.75 | 1.6 × 107 | 5 × 1043 | 1 × 109 | 1.9 × 1013 | 26.13 | -22.89 | Not Detectable | Not Applicable |
15 | 6.4 | 0.13 | 6.8 × 105 | 3.9 × 1040 | 5.7 × 106 | 3.6 × 1011 | 30.86 | -18.16 | 152.63 | 21.46 |
16 | 6.41 | 1.16 | 1.4 × 107 | 3.6 × 1043 | 4.4 × 108 | 1.1 × 1013 | 26.87 | -22.15 | Not Detectable | Not Applicable |
17 | 6.42 | 2.23 | 6.6 × 105 | 3.5 × 1041 | 8.2 × 107 | 1.8 × 1012 | 28.76 | -20.26 | 153.28 | 21.28 |
18 | 6.5 | 0.04 | 4.7 × 107 | 3.3 × 1043 | 4.8 × 108 | 1.1 × 1013 | 26.88 | -22.18 | Not Detectable | Not Applicable |
19* | 6.5 | 0.17 | 3 × 106 | 1.2 × 1042 | 4.8 × 108 | 1 × 1013 | 27.29 | -21.78 | 26.34 | 720.46 |
20 | 6.51 | 0.67 | 1.2 × 106 | 6.3 × 1041 | 8.8 × 107 | 2.2 × 1012 | 28.91 | -20.16 | 81.70 | 74.91 |
21 | 6.51 | 0.79 | 1.3 × 106 | 7.8 × 1041 | 2 × 107 | 9.1 × 1011 | 30.2 | -18.87 | 72.44 | 95.28 |
22 | 6.51 | 0.88 | 4 × 106 | 6.4 × 1042 | 1.2 × 108 | 1.3 × 1012 | 28.51 | -20.55 | Not Detectable | Not Applicable |
23 | 6.55 | 1.23 | 1.5 × 107 | 3.5 × 1043 | 8.5 × 108 | 1.6 × 1013 | 26.45 | -22.61 | Not Detectable | Not Applicable |
24 | 6.6 | 0.31 | 6.8 × 105 | 1.7 × 1041 | 6.3 × 107 | 1.8 × 1012 | 28.9 | -20.20 | 147.28 | 23.05 |
25 | 6.61 | 0.28 | 1.4 × 107 | 6.4 × 1043 | 5.8 × 108 | 1.2 × 1013 | 26.33 | -22.77 | Not Detectable | Not Applicable |
26 | 6.68 | 0.71 | 1.8 × 108 | 1.2 × 1044 | 4.8 × 108 | 9.7 × 1012 | 25.87 | -23.27 | Not Detectable | Not Applicable |
27 | 6.69 | 0.45 | 6.8 × 105 | 1.1 × 1040 | 9 × 106 | 4.7 × 1011 | 30.96 | -18.18 | 145.09 | 23.75 |
28 | 6.7 | 0.07 | 6.9 × 105 | 7.5 × 1039 | 6.1 × 106 | 3.9 × 1011 | 31.08 | -18.06 | 144.11 | 24.08 |
29 | 6.76 | 1.4 | 1 × 107 | 4.2 × 1043 | 4.8 × 108 | 8.8 × 1012 | 26.79 | -22.39 | Not Detectable | Not Applicable |
30 | 6.79 | 0.40 | 6.9 × 105 | 8 × 1038 | 2.3 × 106 | 1.6 × 1011 | 32.42 | -16.76 | 142.15 | 24.74 |
31* | 6.8 | 0.27 | 1.5 × 106 | 2 × 1042 | 4.6 × 108 | 6.8 × 1012 | 27.28 | -21.90 | 56.30 | 157.75 |
32 | 6.91 | 0.68 | 1.5 × 106 | 4.5 × 1041 | 3.3 × 108 | 6.1 × 1012 | 27.57 | -21.64 | 94.08 | 56.49 |
33 | 6.92 | 0.88 | 7.1 × 105 | 7.3 × 1039 | 1.4 × 107 | 5.7 × 1011 | 30.5 | -18.72 | 137.90 | 26.29 |
34 | 6.96 | 2.71 | 1.4 × 106 | 6.3 × 1041 | 5.7 × 107 | 1.3 × 1012 | 29.34 | -19.91 | 62.59 | 127.61 |
35 | 6.98 | 1.80 | 7.8 × 105 | 9.6 × 1040 | 2.3 × 107 | 8.4 × 1011 | 30.02 | -19.23 | 132.05 | 28.67 |
36* | 7.01 | 0.65 | 1.1 × 106 | 4 × 1041 | 6.9 × 107 | 2.1 × 1012 | 29.13 | -20.12 | 96.34 | 53.87 |
37 | 7.04 | 2.49 | 1.3 × 107 | 2 × 1043 | 3.5 × 108 | 9.1 × 1012 | 27.52 | -21.73 | Not Detectable | Not Applicable |
38 | 7.2 | 0.15 | 1.2 × 107 | 3.9 × 1043 | 4.2 × 108 | 8.7 × 1012 | 27.13 | -22.19 | Not Detectable | Not Applicable |
39 | 7.24 | 1.32 | 1.2 × 106 | 2.2 × 1042 | 5 × 107 | 1.2 × 1012 | 29.33 | -19.99 | 84.97 | 69.25 |
40 | 7.24 | 2.19 | 2.2 × 106 | 1.5 × 1042 | 2 × 108 | 2.5 × 1012 | 28.25 | -21.07 | 19.22 | 1352.89 |
41 | 7.32 | 1.33 | 7.3 × 105 | 5.4 × 1038 | 4.4 × 107 | 9 × 1011 | 29.45 | -19.90 | 128.22 | 30.41 |
42 | 7.36 | 1.28 | 3.5 × 106 | 2.4 × 1042 | 2.7 × 108 | 4.1 × 1012 | 28.01 | -21.38 | Not Detectable | Not Applicable |
43 | 7.4 | 0.09 | 7.4 × 105 | 4 × 1040 | 3 × 107 | 8.8 × 1011 | 29.57 | -19.82 | 126.26 | 31.36 |
44 | 7.48 | 0.61 | 7.5 × 105 | 4.6 × 1039 | 4.7 × 107 | 1.4 × 1012 | 29.31 | -20.12 | 123.98 | 32.53 |
45 | 7.48 | 0.72 | 7.5 × 105 | 3 × 1039 | 5.7 × 105 | 8.1 × 1010 | 32.88 | -16.54 | 124.48 | 32.27 |
46 | 7.53 | 1.41 | 1.8 × 106 | 9.8 × 1041 | 1.4 × 108 | 2.1 × 1012 | 28.59 | -20.83 | 37.11 | 363.07 |
47 | 7.58 | 0.52 | 7.6 × 105 | 2.9 × 1040 | 1.1 × 107 | 4.4 × 1011 | 30.68 | -18.78 | 121.53 | 33.86 |
48 | 7.62 | 1.05 | 1.1 × 107 | 2.3 × 1043 | 5.3 × 108 | 8.2 × 1012 | 27.39 | -22.07 | Not Detectable | Not Applicable |
49 | 7.75 | 1.18 | 7.9 × 105 | 3.7 × 1040 | 2.9 × 107 | 8.8 × 1011 | 29.86 | -19.66 | 117.33 | 36.32 |
50 | 7.9 | 0.19 | 3.3 × 107 | 4.3 × 1043 | 5.2 × 108 | 7.2 × 1012 | 27.2 | -22.36 | Not Detectable | Not Applicable |
51 | 7.98 | 0.79 | 1.1 × 106 | 8.9 × 1040 | 6 × 106 | 3.2 × 1011 | 31.41 | -18.18 | 87.25 | 65.69 |
52* | 8 | 0.01 | 2.7 × 106 | 8.8 × 1042 | 4.1 × 108 | 4.1 × 1012 | 27.62 | -21.96 | 10.65 | 4408.89 |
53 | 8.01 | 0.39 | 8.7 × 105 | 1.7 × 1040 | 1.6 × 107 | 6.1 × 1011 | 30.68 | -18.90 | 108.16 | 42.74 |
54 | 8.02 | 0.52 | 8 × 105 | 1.9 × 1040 | 1.6 × 107 | 6.1 × 1011 | 30.3 | -19.28 | 112.29 | 39.66 |
55 | 8.51 | 0.29 | 1.2 × 106 | 1.5 × 1041 | 2.3 × 107 | 7.1 × 1011 | 30.16 | -19.58 | 75.95 | 86.69 |
56 | 8.99 | 0.07 | 9 × 105 | 4.3 × 1040 | 3.2 × 107 | 6.3 × 1011 | 30.0 | -19.88 | 93.90 | 56.71 |
Notes. In this table, for each GW event (first column) associated with a host galaxy in the AGN_fid case, we report the redshift of the merger (second column), the distance between the primary BH and the associated galaxy (third column), the chirp mass (fourth column), the X-ray (fifth column), [CII] (sixth column) and FIR (seventh column) luminosities in solar units, the apparent and absolute UV magnitudes (eighth and ninth column), the S/N (tenth column) and the angular resolution (eleventh column). We show the cases with either significant S/N or significant brightness in different EM bands.
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