Table B.1
.Fitted parameters for the redshift evolution of DM median, wDM,rf, and wRM,rf.
| median DMhost,rf fit | wDM,rf fit | wRM,rf fit | ||||||||
|---|---|---|---|---|---|---|---|---|---|---|
| a | b | c | a | b | c | ARM | DRM | BRM | CRM | |
| All galaxies | 82 ± 4 | 0.8 ± 0.1 | 40 ± 3 | 241 ± 40 | 0.6 ± 0.1 | 93 ± 34 | 267 ± 4 | 1.24 ± 0.04 | −0.57 ± 0.03 | 117 ± 3 |
| Star-forming | 81 ± 4 | 0.8 ± 0.1 | 43 ± 3 | 113 ± 8 | 0.7 ± 0.1 | 94 ± 7 | 264 ± 4 | 1.24 ± 0.04 | −0.57 ± 0.03 | 125±3 |
| Red | 41 ± 3 | 1.4± 0.1 | 13 ± 2 | 82 ± 7 | 1.3 ± 0.1 | 33 ± 4 | 60 ± 17 | 20.41 ± 304.02 | −24.0 ± 433.73 | 38 ± 7 |
| 9 <log(M*/M⊙)< 9.5 | 70 ± 3 | 0.74± 0.05 | 41 ± 3 | 95 ± 6 | 0.7 ± 0.1 | 87 ± 5 | 155 ± 4 | 1.16 ± 0.07 | −0.47 ± 0.05 | 111 ± 3 |
| 9.5 <log(M*/M⊙)< 10 | 83 ± 4 | 0.78 ± 0.05 | 50 ± 3 | 107 ± 8 | 0.7 ± 0.1 | 105 ± 7 | 280 ± 8 | 1.1 ± 0.07 | −0.44 ± 0.05 | 151 ± 6 |
| 10 <log(M*/M⊙)< 10.5 | 97 ± 5 | 0.7 ± 0.05 | 47 ± 4 | 121 ± 8 | 0.6 ± 0.1 | 121 ± 6 | 484 ± 20 | 1.04 ± 0.1 | −0.49 ± 0.07 | 155 ± 17 |
| 10.5 <log(M*/M⊙)< 11 | 105 ± 8 | 0.97 ± 0.08 | 18 ± 6 | 188 ± 15 | 0.7 ± 0.1 | 56 ± 12 | 530 ± 20 | 2.32 ± 0.19 | −0.94 ± 0.1 | 76 ± 12 |
| 11 < log(M*/M⊙) < 12 | 79 ± 6 | 1.35 ± 0.09 | 26 ± 4 | 168 ± 18 | 1.2 ± 0.1 | 52 ± 12 | 293 ± 27 | 3.4 ± 0.65 | −2.02 ± 0.41 | 62 ± 15 |
| i < 10° | 65 ± 2 | 0.93 ± 0.03 | 33 ± 1 | 94 ± 5 | 0.9 ± 0.1 | 62 ± 4 | 171 ± 3 | 1.38 ± 0.05 | −0.43 ± 0.03 | 56 ± 2 |
| 10° < i < 45° | 70 ± 2 | 0.87 ± 0.04 | 35 ± 2 | 98 ± 5 | 0.9 ± 0.1 | 67 ± 4 | 202 ± 2 | 1.35 ± 0.03 | −0.48 ± 0.02 | 77 ± 2 |
| 45° < i < 80° | 86 ± 5 | 0.73 ± 0.05 | 42 ± 4 | 117 ± 8 | 0.7 ± 0.1 | 95 ± 7 | 291 ± 4 | 1.22 ± 0.04 | −0.6 ± 0.03 | 130 ± 4 |
| 80° < i | 94 ± 7 | 0.63 ± 0.07 | 48 ± 6 | 124 ± 15 | 0.4 ± 0.1 | 142 ± 14 | 333 ± 8 | 1.11 ± 0.07 | −0.67 ± 0.05 | 184± 7 |
| boffset < 5 kpc | 78 ± 2 | 0.84± 0.02 | 50 ± 1 | 96 ± 5 | 0.67 ± 0.05 | 112±4 | 301 ± 3 | 1.16 ± 0.03 | −0.33 ± 0.02 | 201 ± 2 |
| 5 kpc < boffset < 10 kpc | 86 ± 7 | 0.72 ± 0.08 | 38 ± 6 | 121 ± 10 | 0.69 ± 0.08 | 86 ± 9 | 253 ± 6 | 1.3 ± 0.07 | −0.7 ± 0.05 | 92 ± 5 |
| 10 kpc < boffset < 30 kpc | 82 ± 7 | 0.7 ± 0.08 | 30 ± 6 | 135 ± 14 | 0.64 ± 0.09 | 68 ± 12 | 166 ± 6 | 1.18 ± 0.1 | −0.72 ± 0.07 | 59 ± 5 |
| 30 kpc < boffset | 52 ± 2 | 1.18 ± 0.05 | 30 ± 1 | 136 ± 13 | 0.88 ± 0.1 | 55 ± 10 | 37 ± 5 | 0.99 ± 0.32 | 0.0 ± 0.17 | 27 ± 4 |
Notes. This table shows information for the actual rest frame DMhost and RMhost distributions (without fitting). The DM median and 1σ width (wDM,rf) is fitted by a power law, and the RM 1σ width (wRM,rf) by a curved power law as a function of redshift. The different lines of the table correspond to using every galaxy, galaxies with different star formation activity, galaxies in different stellar mass bins, galaxies with different inclinations and FRBs with different projected offsets from the center of the host galaxy (boffset). We also list the fitted parameters of the curved power law relation between the width of the actual RM distribution (without fitting) and redshift for the same subsets of galaxies.
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