Table A.1.
Host galaxy candidates and association probability for FRBs with ≤5 galaxies within the error region.
| FRB | ID | Galaxy name | zphot | rr (") | mr | P(O) | P(O|x) |
|---|---|---|---|---|---|---|---|
| FRB 20200210A | G1 | PSO J283.5110+46.3322 | 0.11 ± 0.01 | 6.1 | 18.0 | 0.924 | 0.580 |
| G2 | PSO J283.5087+46.3348 | 0.40 ± 0.08 | 3.3 | 21.0 | 0.040 | 0.003 | |
| G3 | PSO J283.5028+46.3205 | 0.46 ± 0.06 | 2.9 | 21.5 | 0.025 | 0.289 | |
| U | 0.01 | 0.129 | |||||
| FRB 20200216A | G1 | PSO J332.0996+16.6087 | 0.49 ± 0.07 | 2.6 | 21.4 | 0.325 | 0.424 |
| G2 | PSO J332.0953+16.5341 | 0.51 ± 0.20 | 2.5 | 22.3 | 0.138 | 0.004 | |
| G3 | PSO J332.1018+16.6091 | 0.52 ± 0.09 | 2.4 | 21.6 | 0.265 | 0.370 | |
| G4 | PSO J332.0976+16.5926 | 0.56 ± 0.32 | 2.4 | 22.1 | 0.171 | 0.139 | |
| U | 0.1 | 0.064 | |||||
| FRB 20200419A | G1 | PSO J285.2463+81.7361 | 0.15 ± 0.03 | 3.5 | 19.6 | 0.999 | 0.704 |
| U | 0.001 | 0.296 | |||||
| FRB 20200518A | G1 | PSO J144.1948+77.3261 | 0.08 ± 0.03 | 4.6 | 19.9 | 0.350 | 0.415 |
| G2 | PSO J144.2179+77.3481 | 0.08 ± 0.02 | 4.6 | 19.4 | 0.640 | 0.557 | |
| U | 0.01 | 0.028 | |||||
| FRB 20200719A | G1 | PSO J139.6135+77.4537 | 0.81 ± 0.96 | 2.4 | 22.7 | 0.048 | 1.8 × 10−4 |
| G2 | PSO J139.6677+77.3898 | 1.45 ± 0.51 | 3.7 | 22.6 | 0.052 | 0.101 | |
| U | 0.9 | 0.899 | |||||
| FRB 20210317A | G1 | PSO J294.1082+59.8453 | 0.15 ± 0.05 | 3.2 | 20.0 | 0.391 | 0.541 |
| G2 | PSO J294.1097+59.8285 | 0.15 ± 0.06 | 4.5 | 19.9 | 0.412 | 0.350 | |
| G3 | PSO J294.1028+59.8412 | 0.30 ± 0.05 | 2.4 | 20.7 | 0.186 | 0.088 | |
| U | 0.01 | 0.021 | |||||
| FRB 20211024B | G1 | PSO J200.1431+42.4925 | 0.24 ± 0.07 | 2.9 | 20.5 | 0.194 | 0.235 |
| G2 | PSO J200.1445+42.4911 | 0.24 ± 0.02 | 5.2 | 19.4 | 0.604 | 0.609 | |
| G3 | PSO J200.1529+42.5097 | 0.34 ± 0.35 | 1.0 | 24.5 | 0.006 | 3.3 × 10−4 | |
| G4 | PSO J200.1548+42.5192 | 0.56 ± 0.27 | 2.7 | 21.8 | 0.052 | 4.2 × 10−4 | |
| G5 | PSO J200.1392+42.4859 | 0.58 ± 0.18 | 1.9 | 22.0 | 0.045 | 0.042 | |
| U | 0.1 | 0.113 | |||||
Notes. The galaxies are sorted by increasing redshift. Their ID is the same identifier as used in the text. The galaxy name is given by the Pan-STARRS source catalogue. The photometric redshift and errors are given by PS1-STRM. rr and mr are respectively the Kron radius and the magnitude in the r band as given by Pan-STARRS. P(O) and P(O|x) are respectively the PATH prior and posterior probability that the galaxy is associated with the FRB. For each FRB, U represents the unseen galaxies.
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