Table 6
ALERT FRBs up to 2019 Dec 31.
| FRB | Internal | MJD | S/N | DM | DMmw | zmax | Width | Fluence | RA | Dec |
|---|---|---|---|---|---|---|---|---|---|---|
| name | (pc cm−3) | (pc cm−3) | (ms) | (Jy ms) | (J2000) | (J2000) | ||||
| 20190709A | 190709 | 58673.21792057 | 26 | 663.1±0.1 | 52 / 45 | 0.65 | 0.49±0.05 | 7.0±1.4 | 01:39:19s | +32:03:13 |
| 190903 w | 58729.02228880 | 8 | 664±10 | 53 / 46 | 0.65 | 23±2 | 98±20 | 01:32:47 | +33:03:43 | |
| 20190926B | 190925 | 58752.03093855 | 15 | 957.3±0.5 | 51 / 44 | 0.97 | 2.2±0.2 | 7.6±1.5 | 01:42:06 | +30:58:05 |
| 20191020B | 191020 | 58776.78080366 | 17 | 465.0±0.2 | 102 / 101 | 0.38 | 1.04±0.10 | 9.1±1.8 | 20:30:39 | +62:17:43 |
| 20191108A(M) | 191108 | 58795.83082563 | 103 | 588.1±0.1 | 43 / 52 | 0.54 | 0.34±0.03 | 8.2±1.6 | 01:33:47 | +31:51:30 |
| 20191109A | 191109 | 58796.54885262 | 22 | 531.2±0.1 | 108 /108 | 0.44 | 0.48±0.05 | 4.5±0.9 | 20:35:15 | +61:49:02 |
Notes. First column lists TNS name, second lists previously used name (cf. Oostrum et al. 2020; Connor et al. 2020; Oostrum 2020b). MJD refers to the arrival time at the solar system barycentre at infinite frequency. DMs and widths were measured with pdmp from psrchive (Hotan et al. 2004). DMMW are the Milky Way DMs predicted using the NE2001 (Cordes & Lazio 2002) and YMW16 (Yao et al. 2017) models, respectively. We assume a 10% uncertainty on the observed pulse widths and 20% on the derived fluences. The position error regions are strongly elongated and presented individually. The best position is not always at the centre of the elliptical region. The derivation of the redshift upper limit zmax is described in Sect. 10.4. (*)Candidate (**)The arrival time published in Connor et al. (2020) contained an error in the barycentric correction. In this table that is rectified.
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