GCN Circular 34127

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

We identified the compact binary merger candidate S230630bq during
real-time processing of data from LIGO Hanford Observatory (H1) and
LIGO Livingston Observatory (L1) at 2023-06-30 23:45:32.407 UTC (GPS
time: 1372203950.407). The candidate was found by the MBTA [1], GstLAL
[2], PyCBC Live [3], and SPIIR [4] analysis pipelines.

S230630bq is an event of interest because its false alarm rate, as
estimated by the online analysis, is 7.7e-09 Hz, or about one in 4
years. The event's properties can be found at this URL:

https://gracedb.ligo.org/superevents/S230630bq

The classification of the GW signal, in order of descending
probability, is BBH (97%), Terrestrial (3%), 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%. [5] Using the masses and spins inferred from the
signal, the probability of matter outside the final compact object
(HasRemnant) is <1%. [5] 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 8%.

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 [6], distributed via GCN notice about 33 seconds after the
candidate event time.
 * bayestar.multiorder.fits,2, an initial localization generated by
BAYESTAR [6], 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
1976 deg2. Marginalized over the whole sky, the a posteriori
luminosity distance estimate is 1150 +/- 360 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] Aubin et al. CQG 38, 095004 (2021)
 [2] Tsukada et al. arXiv:2305.06286
Not found
 
 
 (2023) and Ewing et al.
arXiv:2305.05625
Not found
 
 
 (2023)
 [3] Dal Canton et al. ApJ 923, 254 (2021)
 [4] Chu et al. PRD 105, 024023 (2022)
 [5] Chatterjee et al. ApJ 896, 54 (2020)
 [6] Singer & Price PRD 93, 024013 (2016)