TITLE:   GCN CIRCULAR
NUMBER:  41058
SUBJECT: LIGO/Virgo/KAGRA S250629bs: Upper limits from Swift/BAT-GUANO
DATE:    25/07/10 14:47:59 GMT
FROM:    Maia Williams at PSU <mjw6837@psu.edu>

Maia Williams (PSU), Samuele Ronchini (PSU), Gayathri Raman (PSU), James DeLaunay (PSU), Tyler Parsotan (NASA GSFC), Jamie A. Kennea (PSU), Aaron Tohuvavohu (Caltech) report:

Swift/BAT was observing 86.28% of the GW localization probability ([Bilby.multiorder.fits](https://gracedb.ligo.org/api/superevents/S250629bs/files/Bilby.multiorder.fits)) at merger time. A fraction 64.89% of the GW localization posterior is contained inside the BAT coded FoV.

The LVK notice, distributed in near real-time, triggered the Swift Mission Operations Center operated Gamma-ray Urgent Archiver for Novel Opportunities (GUANO; [Tohuvavohu et al. 2020, ApJ, 900, 1](https://iopscience.iop.org/article/10.3847/1538-4357/aba94f)).

Upon trigger by this notice, GUANO sent a command to the Swift Burst Alert Telescope (BAT) to save 200 seconds of BAT event-mode data from [-50,+150] seconds around the time of the burst. All the requested event mode data was delivered to the ground.

Using the NITRATES analysis ([DeLaunay + Tohuvavohu 2022, ApJ, 941, 169](https://iopscience.iop.org/article/10.3847/1538-4357/ac9d38)), we searched for emission on 8 timescales from 0.128s to 16.384s in the interval [-20,+20] seconds around the merger time. We find no evidence for a signal, and derive the following upper limits.

We quote the 5-sigma flux upper limits in the 15-350 keV band, weighted over the GW localization, for four spectral templates (soft, normal, and hard GRB-like templates described in [arXiv:1612.02395], and spectral shape from GRB170817A [arXiv:1710.05446]) and for four time bins.
In units of 10^-7 erg/s/cm^2:

|time_bin (s) |soft  |normal|hard  |GRB170817
|-|-|-|-|-|
|0.256        |3.65  |3.14  |2.87  |3.39  
|1.024        |1.87  |1.61  |1.47  |1.74  
|4.096        |1.02  |0.88  |0.80  |0.95  
|16.384       |0.65  |0.56  |0.51  |0.60  


The upper limits as function of sky position are plotted here, alongside the GW localization:
https://zenodo.org/records/15843754

The solid and dashed lines indicate the 90% and 50% GW contour levels, respectively. The corresponding fits file is also included.

GUANO is a fully autonomous, extremely low latency, spacecraft commanding pipeline designed for targeted recovery of BAT event mode data around the times of compelling astrophysical events to enable more sensitive GRB searches.

A live reporting of Swift/BAT event data recovered by GUANO can be found at: https://www.swift.psu.edu/guano/