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GCN Circular 36429

Subject

LIGO/Virgo/KAGRA S240511i: Updated Sky localization

Date

2024-05-11T18:17:34Z (3 months ago)

From

Lorenzo Pompili at Max Planck Institute for Gravitational Physics <lorenzo.pompili@aei.mpg.de>

Via

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

We have conducted further analysis of the LIGO Hanford Observatory (H1), LIGO Livingston Observatory (L1), and Virgo Observatory (V1) data around the time of the compact binary merger (CBC) candidate S240511i (GCN Circular 36425Not found
 
 
). 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/S240511i

For the Bilby.multiorder.fits,0 sky map, the 90% credible region is well fit by an ellipse with an area of 89 deg2 described by the following DS9 region (right ascension, declination, semi-major axis, semi-minor axis, position angle of the semi-minor axis):
   icrs; ellipse(11h14m, -18d51m, 12.19d, 2.33d, 112.83d)
Marginalized over the whole sky, the a posteriori luminosity distance estimate is 1906 +/- 404 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/.

 [1] Ashton et al. ApJS 241, 27 (2019) doi:10.3847/1538-4365/ab06fcNot found
 
 
 and Morisaki et al. (2023) arXiv:2307.13380Not found