Table A.5.
Upper limits on the γ-to-radio luminosity ratio, Lγ, 1 ms/Lradio.
| FRB | νradio | Fradio | Lradio | log(Lγ, 1 ms/Lradio) |
|---|---|---|---|---|
| (GHz) | (Jy) | (erg s−1) | ||
| 170712 | 1.297 | 37.8 | 1.0 × 1045 | 7.4 |
| 170906 | 1.297 | 29.6 | 1.0 × 1045 | 7.9 |
| 171003 | 1.297 | 40.5 | 1.7 × 1045 | 7.1 |
| 171004 | 1.297 | 22.0 | 5.8 × 1044 | 7.6 |
| 171019 | 1.297 | 40.5 | 1.7 × 1045 | 7.0 |
| 171116 | 1.297 | 19.6 | 1.1 × 1045 | 7.7 |
| 171209 | 1.352 | 1.48 | 1.8 × 1044 | 8.6 |
| 171213 | 1.297 | 88.6 | 8.6 × 1044 | 7.2 |
| 171216 | 1.297 | 21.0 | 3.3 × 1044 | 7.4 |
| 180110 | 1.297 | 128.1 | 8.4 × 1045 | 6.5 |
| 180119 | 1.297 | 40.7 | 1.5 × 1045 | 7.4 |
| 180128.0 | 1.297 | 17.5 | 7.2 × 1044 | 7.8 |
| 180128.2 | 1.297 | 28.7 | 1.3 × 1045 | 7.7 |
| 180131 | 1.297 | 22.2 | 1.3 × 1045 | 7.5 |
| 180301 | 1.352 | 1.30 | 5.0 × 1043 | 8.5 |
| 180311 | 1.352 | 0.15 | 2.1 × 1043 | 9.9 |
| 180430 | 1.297 | 147.5 | 1.0 × 1045 | 7.0 |
| 180515 | 1.320 | 24.2 | 7.9 × 1044 | 8.1 |
| 180525 | 1.297 | 78.9 | 2.8 × 1045 | 7.2 |
| 180528 | 0.835 | 15.75 | 8.1 × 1044 | 8.0 |
| 180714 | 1.352 | 0.6 | 7.4 × 1043 | 9.4 |
| 180729.J0558+56 | 0.600 | 112.5 | 1.1 × 1045 | 7.4 |
| 180730.J0353+87 | 0.600 | 119.0 | 4.2 × 1045 | 7.4 |
| 180810.J0646+34 | 0.600 | 40.74 | 5.8 × 1044 | 7.5 |
| 180810.J1159+83 | 0.600 | 60.71 | 2.8 × 1044 | 7.3 |
| 180817.J1533+42 | 0.600 | 70.27 | 3.0 × 1045 | 7.5 |
| 180916.J0158+65 | 0.600 | 1.64 | 2.8 × 1040 | 9.0 |
| 180923 | 1.352 | 2.90 | 1.5 × 1044 | 9.0 |
| 180924 | 1.320 | 12.3 | 5.8 × 1043 | 8.0 |
| 181017 | 0.835 | 161. | 2.0 × 1045 | 7.2 |
| 181030.J1054+73 | 0.600 | 12.37 | 2.0 × 1042 | 8.5 |
| 181119.J12+65 | 0.600 | 0.29 | 4.4 × 1042 | 10.1 |
| 181228 | 0.835 | 19.23 | 3.6 × 1044 | 7.9 |
| 190116.J1249+27 | 0.600 | 0.2 | 3.9 × 1042 | 10.1 |
| 190209.J0937+77 | 0.600 | 0.54 | 9.5 × 1042 | 9.5 |
| 190523 | 1.411 | 667 | 1.9 × 1046 | 6.3 |
| 190711 | 0.835 | 6.7 (a) | 2.3 × 1044 | 8.1 |
| 190714 | 1.297 | 8.0 (a) | 3.7 × 1044 | 7.7 |
| 190806 | 0.835 | 3.9 | 9.0 × 1043 | 8.4 |
Notes. Radio data (central frequency, flux density), radio luminosity calculated as Lradio = ν Lν are also reported. Radio luminosities were calculated assuming the same redshift limits or values for the γ-ray ones, so their ratio does not depend on z. For the FRBs for which the flux density is not reported in frbcat, we estimated it from the fluence density and the burst width.
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