GCN Circular 34785

The LIGO Scientific Collaboration, the Virgo Collaboration, and the
KAGRA Collaboration report:

We identified the compact binary merger candidate S231001aq during
real-time processing of data from LIGO Hanford Observatory (H1) and
LIGO Livingston Observatory (L1) at 2023-10-01 14:02:20.720 UTC (GPS
time: 1380204158.720). The candidate was found by the CWB [1], GstLAL
[2], MBTA [3], oLIB [4], PyCBC Live [5], and SPIIR [6] analysis
pipelines.

S231001aq is an event of interest because its false alarm rate, as
estimated by the online analysis, is 5e-09 Hz, or about one in 6
years. The event's properties can be found at this URL:

https://gracedb.ligo.org/superevents/S231001aq

The classification of the GW signal, in order of descending
probability, is BBH (>99%), Terrestrial (<1%), NSBH (<1%), or BNS
(<1%).

Assuming the candidate is astrophysical in origin, the probability
that the lighter compact object is consistent with a neutron star mass
(HasNS) is <1%. [7] Using the masses and spins inferred from the
signal, the probability of matter outside the final compact object
(HasRemnant) is <1%. [7] 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,1, an initial localization generated by
BAYESTAR [8], distributed via GCN notice about 31 seconds after the
candidate event time.
 * bayestar.multiorder.fits,2, an initial localization generated by
BAYESTAR [8], distributed via GCN notice about 5 minutes after the
candidate event time.

The preferred sky map at this time is bayestar.multiorder.fits,2. For
the bayestar.multiorder.fits,2 sky map, the 90% credible region is
4091 deg2. Marginalized over the whole sky, the a posteriori
luminosity distance estimate is 1569 +/- 465 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
https://emfollow.docs.ligo.org/userguide/.

 [1] Klimenko et al. PRD 93, 042004 (2016)
 [2] Tsukada et al. arXiv:2305.06286
Not found
 
 
 (2023) and Ewing et al.
arXiv:2305.05625
Not found
 
 
 (2023)
 [3] Aubin et al. CQG 38, 095004 (2021)
 [4] Lynch et al. PRD 95, 104046 (2017)
 [5] Dal Canton et al. ApJ 923, 254 (2021)
 [6] Chu et al. PRD 105, 024023 (2022)
 [7] Chatterjee et al. ApJ 896, 54 (2020)
 [8] Singer & Price PRD 93, 024013 (2016)