detection in a single fan-beam occurred $\approx20\%$ of the time. The localisation of this FRB is thus slightly poorer ($21\arcsec \times 8.4^{\circ}$) than for the other two FRBs, for which 2 fan-beam detections allow more accurate positions.\

\[tab:specs\]

  ------------------------------------------------------------- ------------------------- ------------------------- -------------------------
                            Parameter                                  FRB 160317                FRB 160410                FRB 160608
                       \[0.5ex\] UTC start                         2016-03-17-08:30:58       2016-04-10-08:16:54       2016-06-08-03:52:24
                            UTC event                            2016-03-17-09:00:36.530   2016-04-10-08:33:39.680   2016-06-08-03:53:01.088
                       RA J2000 (hh:mm:ss)                              07:53:47                  08:41:25                  07:36:42
                      DEC J2000 (dd:mm:ss)                             $-$29:36:31                +06:05:05                $-$40:47:52
                            $l$ (deg)                                    246.05                    220.36                    254.11
                            $b$ (deg)                                    $-$0.99                    27.19                    $-$9.54
                          Detection S/N                                    13                        13                        12
                   $S_\mathrm{peak, obs}$ (Jy)                           $>3.0$                    $>7.0$                    $>4.3$
                    Boresight Fluence (Jyms)                              $>69$                     $>34$                     $>37$
                  Isotropic energy, $E_{0}$ (J)                      $\sim 10^{34}$            $\sim 10^{32}$            $\sim 10^{33}$
                    Observed width, $W$ (ms)                              21(7)                     4(1)                      9(6)
         DM smearing, $\uptau_{843 \,\mathrm{MHz}}$ (ms)                  12.6                       3.0                       7.4
            $\mathrm{DM}_\mathrm{FRB}$ (pc cm$^{-3}$)                   1165(11)                   278(3)                    682(7)
   $\mathrm{DM}_{\mathrm{Gal},\mathrm{NE2001}}$ (pc cm$^{-3}$)            319.6                     57.7                      238.3
   $\mathrm{DM}_{\mathrm{Gal},\mathrm{YMW16}}$ (pc cm$^{-3}$)             394.6                     62.5                      310.3
                     Inferred redshift, $z$                                0.7                       0.2                       0.4
                    Luminosity Distance (Gpc)                             4.30                      0.89                      1.97
                    Co-moving Distance (Gpc)                              2.52                      0.75                      1.44
                        Boresight source                             SGR 0755$-$2933            J0837$+$0610              J0738$-$4042
                             \[1ex\]                                                                                
  ------------------------------------------------------------- ------------------------- ------------------------- -------------------------

The primary advantage of the array is that a pulse from a far-field point source is detected in a maximum of 3 adjacent fan-beams at any given time, confirmed 