Table 3.
Observational and instrumental parameters of FRBs in our sample.
| FRB name | gl | gb | DMobs | S/N | S/Nlim | Fluence | wobs | Flux | z† | Ref. |
|---|---|---|---|---|---|---|---|---|---|---|
| (deg) | (deg) | (pc cm−3) | (Jy ms) | (ms) | (Jy) | |||||
| ASKAP | ||||||||||
| 180525 | 349.0 | 50.7 | 388.1 | 27.4 | 9.5 | 300 | 3.8 | 78.9 | 0.174 |
Ma18 |
| 180324 | 245.2 | –20.5 | 431 | 9.8 | 9.5 | 71 | 4.3 | 16.51 | 0.172 |
Ma18 |
| 180315 | 13.2 | –20.9 | 479 | 10.4 | 9.5 | 56 | 2.4 | 23.34 | 0.215 |
Ma18 |
| 180212 | 338.3 | 50.0 | 167.5 | 18.3 | 9.5 | 96 | 1.81 | 53.04 | 0.022 |
Sh18 |
| 180131 | 0.6 | –50.7 | 657.7 | 13.8 | 9.5 | 100 | 4.5 | 22.22 | 0.420 |
Sh18 |
| 180130 | 5.9 | –51.8 | 343.5 | 10.2 | 9.5 | 95 | 4.1 | 23.17 | 0.132 |
Sh18 |
| 180128.2 | 327.8 | –48.6 | 495.9 | 9.6 | 9.5 | 66 | 2.3 | 28.7 | 0.270 |
Sh18 |
| 180128.0 | 326.7 | 52.2 | 441.4 | 12.4 | 9.5 | 51 | 2.9 | 17.6 | 0.221 |
Sh18 |
| 180119 | 199.5 | –50.4 | 402.7 | 15.9 | 9.5 | 110 | 2.7 | 40.74 | 0.175 |
Sh18 |
| 180110 | 7.8 | –51.9 | 715.7 | 35.6 | 9.5 | 420 | 3.2 | 131.25 | 0.472 |
Sh18 |
| 171216 | 273.9 | –48.4 | 203.1 | 10.3 | 9.5 | 40 | 1.9 | 21.06 | 0.034 |
Sh18 |
| 171213 | 200.6 | –48.3 | 158.6 | 25.1 | 9.5 | 133 | 1.5 | 88.67 | 0.013 |
Sh18 |
| 171116 | 205.0 | –49.8 | 618.5 | 11.8 | 9.5 | 63 | 3.2 | 19.69 | 0.372 |
Sh18 |
| 171020 | 29.3 | –51.3 | 114.1 | 19.5 | 9.5 | 200 | 3.2 | 62.5 | 0.006 |
Sh18 |
| 171019 | 52.5 | –49.3 | 460.8 | 23.4 | 9.5 | 219 | 5.4 | 40.56 | 0.245 |
Sh18 |
| 171004 | 282.2 | 48.9 | 304 | 10.9 | 9.5 | 44 | 2 | 22. | 0.095 |
Sh18 |
| 171003 | 283.4 | 46.3 | 463.2 | 13.8 | 9.5 | 81 | 2 | 40.5 | 0.232 |
Sh18 |
| 170906 | 34.2 | –49.5 | 390.3 | 17 | 9.5 | 74 | 2.5 | 29.6 | 0.173 |
Sh18 |
| 170712 | 329.3 | –51.6 | 312.79 | 12.7 | 9.5 | 53 | 1.4 | 37.86 | 0.109 |
Sh18 |
| 170707 | 269.1 | –50.5 | 235.2 | 9.5 | 9.5 | 52 | 3.5 | 14.86 | 0.053 |
Sh18 |
| 170428 | 359.2 | –49.9 | 991.7 | 10.5 | 9.5 | 34 | 4.4 | 7.73 | 0.716 |
Sh18 |
| 170416 | 337.6 | –50 | 523.2 | 13 | 9.5 | 97 | 5 | 14.4 | 0.293 |
Sh18 |
| 170107 | 266.0 | 51.4 | 609.5 | 16 | 9.5 | 58 | 2.4 | 24.17 | 0.376 |
Ba17 |
| Parkes | ||||||||||
| 160102 | 18.9 | –60.8 | 2596.1 | 16 | 10 | 1.8 | 3.4 | 1.06 | 2.097 |
Bh18 |
| 151230 | 239.0 | 34.8 | 960.4 | 17 | 10 | 1.9 | 4.4 | 0.86 | 0.682 |
Bh18 |
| 151206 | 32.6 | –8.5 | 1909.8 | 10 | 10 | 0.9 | 3 | 0.6 | 1.395 |
Bh18 |
| 150610 | 278.0 | 16.5 | 1593.9 | 18 | 10 | 1.3 | 2 | 0.53 | 1.155 |
Bh18 |
| 150418 | 232.7 | –3.2 | 776.2 | 39 | 10 | 1.76 | 0.8 | 2.2 | 0.247 |
Ke16 |
| 150215 | 24.7 | 5.3 | 1105.6 | 19 | 10 | 2.02 | 2.88 | 0.7 | 0.582 |
Pe17 |
| 140514 | 50.8 | –54.6 | 562.7 | 16 | 10 | 1.32 | 2.82 | 0.47 | 0.331 |
Pe15 |
| 131104 | 260.6 | –21.9 | 779 | 34 | 10 | 2.75 | 2.37 | 1.16 | 0.352 |
Sh16 |
| 130729 | 324.8 | 54.7 | 861 | 14 | 10 | 3.43 | 15.61 | 0.22 | 0.602 |
Ch15 |
| 130628 | 226.0 | 30.7 | 469.88 | 29 | 10 | 1.22 | 0.64 | 1.91 | 0.230 |
Ch15 |
| 130626 | 7.5 | 27.4 | 952.4 | 21 | 10 | 1.47 | 1.98 | 0.75 | 0.648 |
Ch15 |
| 121002 | 308.2 | –26.3 | 1629.18 | 16 | 10 | 2.34 | 5.44 | 0.43 | 1.240 |
Ch15 |
| 120127 | 49.3 | –66.2 | 553.3 | 13 | 9 | 0.75 | 1.21 | 0.62 | 0.331 |
Th13 |
| 110703 | 81.0 | –59.0 | 1103.6 | 17 | 9 | 1.75 | 4.3 | 0.41 | 0.817 |
Th13 |
| 110626 | 355.9 | –41.8 | 723 | 12 | 9 | 0.89 | 1.41 | 0.63 | 0.471 |
Th13 |
| 110220 | 50.8 | –54.8 | 944.38 | 54 | 9 | 7.31 | 6.59 | 1.11 | 0.674 |
Th13 |
| 110214 | 290.7 | –66.6 | 168.9 | 13 | 5 | 51.3 | 1.9 | 27. | 0.022 |
Pe18 |
| 090625 | 226.4 | –60.0 | 899.55 | 30 | 10 | 2.19 | 1.92 | 1.14 | 0.634 |
Ch15 |
| 010621 | 25.4 | -4.0 | 745 | 18 | 8 | 4.24 | 8. | 0.53 | 0.228 |
Pe16 |
| 010125 | 356.6 | –20.0 | 790 | 25 | 7 | 5.72 | 10.6 | 0.54 | 0.495 |
Ke12 |
Notes. ( † )Redshifts z are calculated from DMs as in Sect. 3.
References.
In the last column we report the references for the S/Nlim: Ma18: Macquart et al. (2019); Sh18: Shannon et al. (2018), Ba17: Bannister et al. (2017); Bh18: Bhandari et al. (2018); Ke17: Keane et al. (2016); Pe17: Petroff et al. (2017); Pe15: Petroff et al. (2015); Sh16: Shand et al. (2016); Ch15: Champion et al. (2015); Sc16: Scholz et al. (2016); Th13: Thornton et al. (2013); Pe18: Petroff et al. (2018); ke12: Keane et al. (2012). Parkes FRBs parameters are taken from Petroff et al. (2016) when available, or from the reference in the last column.
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