single pulses from known pulsars.

Results {#sec:results}
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The false positive rate at UTMOST is high due to RFI caused by mobile phone handsets, which produce narrow band (5-MHz) emission in our band, typically in $\approx 20$ ms pulses. These can be eliminated because celestial pulses are expected to be broadband, modulated by a frequency dependent response across the 31.25 MHz bandwidth. This process has been validated using individual pulses from about 20 bright pulsars seen to date. We are presently automating this process using machine learning algorithms, so that pulses can trigger a full voltage dump of the raw data while they are still in the $\approx30$ seconds of ring buffer storage, with alerts issued in near real-time. RFI occurs predominantly at low DM, but the rate is high enough to produce a few hundred spurious candidates above our DM limit of 100 pccm$^{-3}$ daily. Candidates were typically vetted each morning after data taking.

In 2016 March, April and June we made the first interferometric detections of FRBs at 843 MHz: FRB 160317, FRB 160410 and FRB 160608, as shown in Figure \[fig:frbs1\].

FRB 160317
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This was detected on 2016 March 17 at 09:00:36.530 UTC while observing an 