{
  "submitter": "Maria Lisa Brozzetti at Università degli Studi di Perugia  <marialisa.brozzetti@ligo.org>",
  "eventId": "LIGO/Virgo/KAGRA S240910ci",
  "createdOn": 1725970482636,
  "bibcode": "2024GCN.37446....1L",
  "subject": "LIGO/Virgo/KAGRA S240910ci: Identification of a GW compact binary merger candidate",
  "body": "The LIGO Scientific Collaboration, the Virgo Collaboration, and the KAGRA Collaboration report:\n\nWe identified the compact binary merger candidate S240910ci during real-time processing of data from LIGO Hanford Observatory (H1) and LIGO Livingston Observatory (L1) at 2024-09-10 10:35:35.495 UTC (GPS time: 1409999753.495). The candidate was found by the CWB [1], GstLAL [2], MBTA [3], and PyCBC Live [4] analysis pipelines.\n\nS240910ci is an event of interest because its false alarm rate, as estimated by the online analysis, is 3.2e-10 Hz, or about one in 1e2 years. The event's properties can be found at this URL:\n\nhttps://gracedb.ligo.org/superevents/S240910ci\n\nThe initial classification of the GW signal, based on chirp-mass information only [4], in order of descending probability, is BBH (69%), NSBH (31%), Terrestrial (<1%), or BNS (<1%). Preliminary information from parameter estimation seems to indicate a much smaller NSBH probability, and almost certainly a BBH origin.\n\nAssuming 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 9%.\n\nTwo sky maps are available at this time and can be retrieved from the GraceDB event page:\n * bayestar.multiorder.fits,0, an initial localization generated by BAYESTAR [6], distributed via GCN notice about 28 seconds after the candidate event time.\n * bayestar.multiorder.fits,1, an initial localization generated by BAYESTAR [6], distributed via GCN notice about 5 minutes after the candidate event time.\n\nThe preferred sky map at this time is bayestar.multiorder.fits,1. For the bayestar.multiorder.fits,1 sky map, the 90% credible region is 370 deg2. Marginalized over the whole sky, the a posteriori luminosity distance estimate is 641 +/- 169 Mpc (a posteriori mean +/- standard deviation).\n\nFor 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/.\n\n [1] Klimenko et al. PRD 93, 042004 (2016) doi:10.1103/PhysRevD.93.042004\n [2] Tsukada et al. PRD 108, 043004 (2023) doi:10.1103/PhysRevD.108.043004 and Ewing et al. (2023) arXiv:2305.05625\n [3] Aubin et al. CQG 38, 095004 (2021) doi:10.1088/1361-6382/abe913\n [4] Dal Canton et al. ApJ 923, 254 (2021) doi:10.3847/1538-4357/ac2f9a\n [5] Chatterjee et al. ApJ 896, 54 (2020) doi:10.3847/1538-4357/ab8dbe\n [6] Singer & Price PRD 93, 024013 (2016) doi:10.1103/PhysRevD.93.024013\n",
  "submittedHow": "web",
  "circularId": 37446,
  "format": "text/plain"
}