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Table A.1.

Intrinsic properties of GW host galaxies.

Event Number Redshift Distance between galaxy M1 M2 M ˙ $ \boldsymbol{\dot{M}} $ SFR Mstellar Mdust Metallicity
and BH (physical kpc) (M) (M) (M yr−1) (M yr−1) (M) (M) (Z)

1 6 0.48 1.31×106 1.02×105 0.012 13.1 2.02 × 109 1.7 × 106 0.88

2 6 0.08 6.67×108 1×105 37 166 2.53 × 1010 2.5 × 107 0.62

3 6.09 0.51 1.01×105 1×105 1.58×10−5 0.03 1.06×107 9.43×103 0.13

4 6.12 0.59 3.71 × 108 1.03 × 105 11.3 142 2.41 × 1010 2.1 × 107 0.61

5 6.13 3.57 3.82×105 1×105 2.9×10−2 21.9 5.55×109 6.76×106 0.72

6 6.17 4.36 2.17×105 1.01×105 2.9 116 2.1×1010 1.88×107 0.59

7 6.19 0.89 9.86×105 1×105 5.3×10−3 11.3 2.02×109 2.16×106 0.57

8 6.22 1.55 7.58×105 1.04×105 1.37×10−3 9.84 1.18×109 1.31×106 0.75

9 6.22 1.84 2.03×105 1.01×105 2.83×10−2 21.2 5.33×109 6.65×106 0.73

10 6.29 0.82 8.07×105 1.01×105 5.18×10−3 10.9 1.95×109 2.14×106 0.53

11 6.29 0.22 2.37×108 1.0×105 3.42 83.7 1.71×1010 1.46×107 0.56

12 6.3 0.34 4.82×105 1.02×105 1.07×10−2 8.19 1.15×109 1.34×106 0.61

13 6.31 1.08 1.01×105 1×105 1.95×10−5 0.11 1.49×107 1.71×104 0.11

14 6.36 0.75 2.2×108 1.0×105 1.25 59.6 1.2×1010 1.1×107 0.52

15 6.4 0.13 1.09×105 1.01×105 1.82×10−4 1.12 1.71×108 2.06×105 0.29

16 6.41 1.16 1.47×108 1.01×105 0.78 27.1 9.96×109 6.46×106 0.61

17 6.42 2.23 1.03×105 1×105 2.27×10−3 7.72 7.55×108 1.02×106 0.45

18 6.5 0.04 1.39×108 7.84×105 0.72 29.6 9.63×109 6.46×106 0.60

19* 6.5 0.17 1.25×106 2.01×105 9.84×10−3 31.08 4.8×109 5.82×106 0.53

20 6.51 0.67 3.78×105 1.03×105 4.55×10−3 6.96 1.27×109 1.26×106 0.63

21 6.51 0.79 4.33×105 1×105 5.89×10−3 2.06 5.98×108 5.17×105 0.58

22 6.51 0.88 6.66×106 1.0×105 8.32×10−2 8.5 1.11×109 7.49×105 0.72

23 6.55 1.23 1.65×108 1.01×105 0.77 50.46 1.06×1010 9.29×106 0.52

24 6.6 0.31 1.04×105 1.01×105 9.49×10−4 7.31 6.83×108 1.02×106 0.35

25 6.61 0.28 1.45×108 1.0×105 1.72 39.33 7.88×109 7.05×106 0.46

26 6.68 0.71 1.02×108 9.05×106 3.93 33.28 6.95×109 5.46×106 0.46

27 6.69 0.45 1.02×105 1.0×105 4.72×10−5 1.14 1.83×108 2.65×105 0.51

28 6.7 0.07 1.05×105 1.01×105 3.02×10−5 1.02 1.71×108 2.17×105 0.36

29 6.76 1.4 6.41×107 1.0×105 9.84×10−1 33.21 6.38×109 4.99×106 0.47

30 6.79 0.40 1.02×105 1.0×105 2.9×10−6 0.31 8.77×107 9.02×104 0.84

31* 6.8 0.27 5.24×105 1.01×105 1.9×10−2 34.7 2.88×109 3.87×106 0.41

32 6.91 0.68 2.4 × 105 2.1 × 105 0.0031 27.48 2.4 × 109 3.4 × 106 0.38

33 6.92 0.88 1 × 105 1 × 105 3 × 10−5 1.86 2.4 × 108 3.2 × 105 0.41

34 6.96 2.71 4.5 × 105 1 × 105 0.0045 5.55 7.5 × 108 7.1 × 105 0.48

35 6.98 1.80 1.2 × 105 1 × 105 0.0005 2.98 4.2 × 108 4.7 × 105 0.38

36* 7.01 0.65 2.51×105 1.02×105 0.0026 6.77 8.4 × 108 1.2 × 106 0.44

37 7.04 2.49 9.9 × 107 1 × 105 0.38 21.97 7.9 × 109 5.2 × 106 0.65

38 7.2 0.15 8.67×107 1.0×105 0.89 26.35 6.6 × 109 4.9 × 106 0.59

39 7.24 1.32 2.8 × 105 1 × 105 0.021 5.68 5.8 × 108 6.7 × 105 0.38

40 7.24 2.19 1.2 × 106 1 × 105 0.013 16.13 1.5 × 109 1.4 × 106 0.46

41 7.32 1.33 1 × 105 1 × 105 1.9 × 10−6 5.56 3.2 × 108 5.1 × 105 0.33

42 7.36 1.28 3.6 × 106 1 × 105 0.024 21.32 3.2 × 109 2.3 × 106 0.44

43 7.4 0.09 1.02×105 1.01×105 0.00019 5.17 3.5 × 108 5 × 105 0.25

44 7.48 0.61 1.03×105 1.02×105 1.8 × 10−5 6.76 5.3 × 108 8.2 × 105 0.28

45 7.48 0.72 1.01×105 1.01×105 1.2 × 10−5 0.25 3.7 × 107 4.6 × 104 0.18

46 7.53 1.41 6.5 × 105 1 × 105 0.0079 12.99 1.1 × 109 1.2 × 106 0.39

47 7.58 0.52 1.04×105 1.01×105 1.3 × 10−4 1.98 1.7 × 108 2.5 × 105 0.28

48 7.62 1.05 5.3 × 107 1 × 105 0.44 31.52 6.4 × 109 4.6 × 106 0.63

49 7.75 1.18 1 × 105 1 × 105 1.7 × 10−4 4.46 3.3 × 108 5 × 105 0.28

50 7.9 0.19 2.87×107 9.57×105 1 31.32 4.7 × 109 4 × 106 0.6

51 7.98 0.79 2.06×105 1.0×105 4.6×10−4 1.13 1.3×108 1.8×105 0.30

52* 8 0.01 1.49×106 1.02×105 0.13 34.7 2.1 × 109 2.3 × 106 0.36

53 8.01 0.39 1.22×105 1.01×105 7.4 × 10−5 2.22 3.2 × 108 3.4 × 105 0.37

54 8.02 0.52 1.02×105 1.01×105 8.3 × 10−5 3.13 2.6 × 108 3.5 × 105 0.25

55 8.51 0.29 2.18×105 1.01×105 8.60×10−4 4.12 2.35×108 3.80×105 0.25

56 8.99 0.07 1.06×105 1.01×105 2.02×10−4 5.43 2.8×108 3.6×105 0.25

Notes. In this table, for each merger 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 masses of the merging BHs (fourth and fifth column), the accretion rate (in M yr−1) of the merged MBH (sixth column), the star formation rate (in M yr−1, seventh column), the stellar mass (eighth column), the dust mass (ninth column) and the metallicity (tenth column) in solar units.

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