The Astrophysical Journal, 800:81 (16pp), 2015 February 20 Essick et al.
frequency of ∼350 Hz, which corresponds to ∼16
◦
between the
two LIGO detectors and ∼6
◦
between the LIGO’s and Virgo. We
also see that LIB and cWB agree, but LIB’s posterior is “fuzzy,”
which we expect due to template mismatch. The three-detector
network shows similar fringe structures, although now we can
see the main triangulation ring from the two LIGO detectors
modulated by information from Virgo. In the LIB posterior,
we can even see the regular lattice imprinted on neighboring
triangulation rings. We note that the three-detector posteriors are
less similar than the two-detector posteriors, which we discuss
in detail in Sections 4.5 and 5.
Figure 8 is analogous to Figure 7, except it shows data
from BBH injections. For BBH injections, which have wide
bandwidths relative to their central frequencies, we do not expect
fringe peaks. The modulation in the three-detector network
along the single triangulation ring is caused by Virgo. The
cWB posteriors clearly demonstrate the increase in the number
of disjoint regions when progressing from the two-detector
network to the three-detector network.
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