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LIGO/Virgo/KAGRA S230723ac

GCN Circular 34235

Subject
LIGO/Virgo/KAGRA S230723ac: Identification of a GW compact binary merger candidate
Date
2023-07-23T11:55:31Z (2 years ago)
From
ricardo.cabrita@uclouvain.be
The LIGO Scientific Collaboration, the Virgo Collaboration, and the
KAGRA Collaboration report:

We identified the compact binary merger candidate S230723ac during
real-time processing of data from LIGO Hanford Observatory (H1) and
LIGO Livingston Observatory (L1) at 2023-07-23 10:18:34.451 UTC (GPS
time: 1374142732.451). The candidate was found by the, GstLAL
[1], MBTA [2], and SPIIR [3] analysis pipelines.


S230723ac is an event of interest because its false alarm rate, as
estimated by the online analysis, is 5.3e-08 Hz, or about one in 7
months. The event's properties can be found at this URL:

https://gracedb.ligo.org/superevents/S230723ac

The classification of the GW signal, in order of descending
probability, is BBH (87%), Terrestrial (13%), 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%. [4] Using the masses and spins inferred from the
signal, the probability of matter outside the final compact object
(HasRemnant) is <1%. [4] 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 [5], distributed via GCN notice about 25 seconds after the
candidate event time.
 * bayestar.multiorder.fits,1, an initial localization generated by
BAYESTAR [5], 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
1281 deg2. Marginalized over the whole sky, the a posteriori
luminosity distance estimate is 1686 +/- 515 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] Tsukada et al. arXiv:2305.06286 (2023) and Ewing et al. arXiv:2305.05625 (2023)
 [2] Aubin et al. CQG 38, 095004 (2021)
 [3] Chu et al. PRD 105, 024023 (2022)
 [4] Chatterjee et al. ApJ 896, 54 (2020)
 [5] Singer & Price PRD 93, 024013 (2016)


GCN Circular 34245

Subject
LIGO/Virgo/KAGRA S230723ac: Updated Sky localization
Date
2023-07-24T02:22:18Z (2 years ago)
From
Soichiro Morisaki at U. of Tokyo <soichiro.morisaki@ligo.org>
The LIGO Scientific Collaboration, the Virgo Collaboration, and the
KAGRA Collaboration report:

We have conducted further analysis of the LIGO Hanford Observatory
(H1) and LIGO Livingston Observatory (L1) data around the time of the
compact binary merger (CBC) candidate S230723ac (GCN Circular 34235). Parameter estimation has been
performed using Bilby [1] and a new sky map, Bilby.multiorder.fits,0,
distributed via GCN Notice, is available for retrieval from the
GraceDB event page:

https://gracedb.ligo.org/superevents/S230723ac

For the Bilby.multiorder.fits,0 sky map, the 90% credible region is
1117 deg2. Marginalized over the whole sky, the a posteriori
luminosity distance estimate is 1551 +/- 436 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] Ashton et al. ApJS 241, 27 (2019)

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