Table A.4.
Upper limits on the average luminosity of possible γ-ray counterparts as evaluated on a set of different integration times.
| FRB | zmax(a) | L(100 μs) | L(1 ms) | L(10 ms) | L(64 ms) | L(1.024 s) | L(10 s) |
|---|---|---|---|---|---|---|---|
| (1053 | (1052 | (1051 | (1051 | (1050 | (1050 | ||
| erg s−1) | erg s−1) | erg s−1) | erg s−1) | erg s−1) | erg s−1) | ||
| 170712 | 0.6740 | 0.99 | 2.31 | 5.45 | 1.87 | 4.30 | 2.56 |
| 170906 | 0.7500 | 4.35 | 9.25 | 22.60 | 7.65 | 17.50 | 9.96 |
| 171003 | 0.8080 | 1.08 | 2.25 | 5.55 | 1.94 | 4.47 | 2.12 |
| 171004 | 0.6650 | 1.10 | 2.43 | 5.88 | 2.09 | 4.76 | 2.21 |
| 171019 | 0.8080 | 0.85 | 1.86 | 4.57 | 1.63 | 3.83 | 1.73 |
| 171116 | 0.9140 | 2.96 | 6.19 | 15.00 | 5.25 | 11.70 | 6.63 |
| 171209 | 1.2210 | 2.89 | 6.87 | 16.30 | 5.65 | 12.30 | 6.58 |
| 171213 | 0.4390 | 0.58 | 1.42 | 3.44 | 1.17 | 2.70 | 1.18 |
| 171216 | 0.5340 | 0.31 | 0.75 | 1.79 | 0.63 | 1.40 | 0.71 |
| 180110 | 0.9670 | 1.12 | 2.59 | 6.10 | 2.22 | 4.91 | 2.53 |
| 180119 | 0.7620 | 1.39 | 3.40 | 8.21 | 2.87 | 6.36 | 3.17 |
| 180128.0 | 0.7980 | 2.15 | 4.75 | 11.70 | 4.11 | 9.28 | 4.31 |
| 180128.2 | 0.8310 | 2.69 | 6.30 | 15.70 | 5.47 | 12.30 | 5.49 |
| 180131 | 0.9340 | 2.15 | 4.62 | 11.20 | 3.94 | 8.65 | 4.28 |
| 180301 | 0.7660 | 0.75 | 1.60 | 4.01 | 1.39 | 3.08 | 1.49 |
| 180311 | 1.2970 | 7.34 | 16.80 | 39.80 | 13.90 | 30.70 | 16.60 |
| 180430 | 0.3850 | 0.46 | 1.04 | 2.52 | 0.86 | 1.98 | 0.75 |
| 180515 | 0.7230 | 3.98 | 9.21 | 22.60 | 8.16 | 18.00 | 8.29 |
| 180525 | 0.7540 | 2.12 | 4.96 | 12.10 | 4.31 | 9.69 | 4.30 |
| 180528 | 1.0450 | 3.94 | 8.00 | 19.70 | 6.82 | 15.00 | 8.80 |
| 180714 | 1.2260 | 8.39 | 19.20 | 48.40 | 17.10 | 38.30 | 15.30 |
| 180729.J0558+56 | 0.6150 | 1.26 | 2.85 | 7.05 | 2.46 | 5.57 | 2.28 |
| 180730.J0353+87 | 1.0260 | 4.06 | 9.41 | 22.90 | 7.90 | 17.80 | 9.23 |
| 180810.J0646+34 | 0.7110 | 0.81 | 1.86 | 4.54 | 1.57 | 3.50 | 1.64 |
| 180810.J1159+83 | 0.4440 | 0.23 | 0.51 | 1.23 | 0.43 | 0.97 | 0.52 |
| 180817.J1533+42 | 1.1120 | 3.94 | 8.61 | 21.50 | 7.51 | 16.80 | 8.89 |
| 180916.J0158+65 | 0.0337 (b) | 1.3 × 10−3 | 3.1 × 10−3 | 7.3 × 10−3 | 2.5 × 10−3 | 5.5 × 10−3 | 3.0 × 10−3 |
| 180923 | 0.8630 | 6.53 | 14.20 | 34.60 | 12.00 | 27.00 | 13.60 |
| 180924 | 0.3214 (c) | 0.29 | 0.65 | 1.58 | 0.55 | 1.23 | 0.59 |
| 181017 | 0.5870 | 1.33 | 2.85 | 7.20 | 2.58 | 5.71 | 2.41 |
| 181030.J1054+73 | 0.1000 | 0.03 | 0.07 | 0.17 | 0.06 | 0.13 | 0.04 |
| 181119.J12+65 | 0.7300 | 2.29 | 5.09 | 12.20 | 4.38 | 9.70 | 4.13 |
| 181228 | 0.6960 | 1.34 | 2.95 | 7.03 | 2.41 | 5.31 | 3.02 |
| 190116.J1249+27 | 0.8080 | 2.48 | 5.23 | 12.70 | 4.49 | 9.89 | 4.93 |
| 190209.J0937+77 | 0.7720 | 1.26 | 2.89 | 7.30 | 2.60 | 5.71 | 1.93 |
| 190523 | 0.66 (d) | 1.47 | 3.59 | 8.57 | 3.05 | 6.81 | 2.99 |
| 190711 | 0.8860 | 1.11 | 2.62 | 6.55 | 2.24 | 5.20 | 2.27 |
| 190714 | 0.8390 | 0.93 | 2.08 | 5.02 | 1.79 | 4.20 | 1.70 |
| 190806 | 0.7550 | 1.22 | 2.54 | 6.36 | 2.20 | 4.86 | 2.40 |
Notes.
Upper limit on redshift z (95% CL) calculated following the prescriptions of Pol et al. (2019).
Spectroscopic redshift of the host galaxy (Marcote et al. 2020).
Spectroscopic redshift of the host galaxy (Bannister et al. 2019).
Spectroscopic redshift of the host galaxy (Ravi et al. 2019).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.