The LIGO Scientific Collaboration, the Virgo Collaboration, and the
KAGRA Collaboration report:
We identified the compact binary merger candidate S231014r during
real-time processing of data from LIGO Hanford Observatory (H1) and
LIGO Livingston Observatory (L1) at 2023-10-14 04:05:32.990 UTC (GPS
time: 1381291550.990). The candidate was found by the CWB , GstLAL
, MBTA , and PyCBC Live  analysis pipelines.
S231014r is an event of interest because its false alarm rate, as
estimated by the online analysis, is 1e-08 Hz, or about one in 3
years. The event's properties can be found at this URL:
The classification of the GW signal, in order of descending
probability, is BBH (>99%), Terrestrial (<1%), NSBH (<1%), or BNS
Assuming the candidate is astrophysical in origin, the probability
that the lighter compact object is consistent with a neutron star mass
(HasNS) is <1%.  Using the masses and spins inferred from the
signal, the probability of matter outside the final compact object
(HasRemnant) is <1%.  Both HasNS and HasRemnant consider the
support of several neutron star equations of state. The probability
that either of the binary components lies between 3 and 5 solar masses
(HasMassgap) is <1%.
Two sky maps are available at this time and can be retrieved from the
GraceDB event page:
* bayestar.multiorder.fits,0, an initial localization generated by
BAYESTAR , distributed via GCN notice about 29 seconds after the
candidate event time.
* bayestar.multiorder.fits,1, an initial localization generated by
BAYESTAR , distributed via GCN notice about 5 minutes after the
candidate event time.
The preferred sky map at this time is bayestar.multiorder.fits,1. For
the bayestar.multiorder.fits,1 sky map, the 90% credible region is
1807 deg2. Marginalized over the whole sky, the a posteriori
luminosity distance estimate is 2857 +/- 903 Mpc (a posteriori mean
+/- standard deviation).
For further information about analysis methodology and the contents of
this alert, refer to the LIGO/Virgo/KAGRA Public Alerts User Guide
 Klimenko et al. PRD 93, 042004 (2016)
 Tsukada et al. arXiv:2305.06286 (2023) and Ewing et al.
 Aubin et al. CQG 38, 095004 (2021)
 Dal Canton et al. ApJ 923, 254 (2021)
 Chatterjee et al. ApJ 896, 54 (2020)
 Singer & Price PRD 93, 024013 (2016)