X-ray magnetar SGR 0755$-$23, in response to an Astronomers Telegram [@Barthelmy]. The burst occurred about 0.4 degrees East of the magnetar, and was detected $\sim$1$^{\circ}$ off the Galactic plane with a DM of 1165(11) pc cm$^{-3}$. The DM due to the ISM at this sight-line is $\sim320$ pc cm$^{-3}$ from the NE2001 model by [@Cordes] and $\sim395$ pc cm$^{-3}$ from the YMW16 model [@Yao]. The burst with S/N $ \sim 13$, occurred East of the centre of the primary fan-beam of detection (Beam 212) since it appeared weakly in the adjacent fan-beam with S/N $\sim 5$ (Beam 213) as shown in Figure \[fig:frbs2\].

FRB 160410
----------

Similarly to FRB 160317, this FRB was also detected in two adjacent fan-beams (Beam 085 with S/N $\sim 13$ and Beam 084 with S/N $\sim 4$) as seen in Figure \[fig:frbs2\]. A single dispersed pulse was discovered on 2016 April 04 at 08:33:39.680 UTC, in an observation of the pulsar J0837$+$0410 at the telescope’s boresight. This pulsar is so bright that individual pulses were seen from it as the FRB occurred, meaning the flux density scale and bandpass response of the observation were well understood. The FRB was seen $\sim 1^{\circ}$ away from boresight. 