Some more details on the second candidate event (a binary BH 23 +13 merger) are at
https://dcc.ligo.org/public/0123/P15...CBC_Search.pdf
This paper gives a comprehensive summary of the signal processing - very interesting methodolgy. Also interesting that signal strength is now being discussed in audio terms - loudnenss. The paper points out the fundamental problem in determining noise statistics in this task - there is no way to isolate the system from GW signals and just look at noise (nothing can shield against GWs).
"Both analyses reported a candidate event on October 12, 2015 at 09:54:43 UTC as the second-loudest event in the observation period,
which we refer to as LVT151012. This candidate event has
a combined matched-filter SNR of 9.6. The PyCBC analysis
reported a false alarm rate of 1 per 2.3 years and a corresponding
false alarm probability of 0.02 for this event. The
GstLAL analysis reported a false alarm rate of 1 per 1.1 years
and a false alarm probability of 0.05. These results are consistent
with expectations for candidate events with low matched-
filter SNR, since PyCBC and GstLAL use different ranking
statistics and background estimation methods. Detector characterization
studies have not identified an instrumental or environmental
artifact as causing this candidate event [14], however
its false alarm probability is not sufficiently low to con-
fidently claim the event as a signal. It is significant enough
to warrant follow-up, however. The results of signal parameter
estimation, shown in Table I, indicate that if LVT151012
is of astrophysical origin, then the source would be a stellarmass
binary black hole system with source-frame component
masses 23+18
−5 M and 13+4
−5 M. The effective spin would be
χeff = 0.0
+0.3
−0.2
and the distance 1100+500
−500 Mpc.