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GRB 241115C

GCN Circular 38245

Subject
GRB 241115C: Swift/BAT-GUANO localization skymap of a burst
Date
2024-11-15T20:45:18Z (6 months ago)
From
Samuele Ronchini at PSU <sjs8171@psu.edu>
Via
Web form
Samuele Ronchini (PSU), James DeLaunay (PSU), Aaron Tohuvavohu (Caltech), Gayathri Raman (PSU), Jamie A. Kennea (PSU), Tyler Parsotan (NASA GSFC) report: 

Swift/BAT did not localize GRB 241115C onboard (T0: 2024-11-15T04:35:33.96 UTC, Fermi trig 753338138) 

The Fermi 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). 

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. 

The BAT likelihood search, NITRATES (DeLaunay + Tohuvavohu 2022, ApJ, 941, 169), performed on the temporal window [T0-20 s, T0+20 s], detects the burst with a sqrt(TS) of 14.65 in a 2.048 s analysis time bin, starting at T0 - 0.5119 s. 

Using the NITRATES analysis, parameter estimation was performed to obtain the localization of this burst in the form of a HEALPIX Multi-Order Coverage (MOC) skymap. This localization accounts for both statistical and systematic errors. More details in the creation and calibration of these maps will soon be published (DeLaunay et al. 2024. in prep)

The 90% credible area is 2,129 deg2 and the 50% credible area is 416 deg2.
The integrated probability inside the coded field of view is 1%. 

The NITRATES skymap is consistent with the Fermi localization reported in the final position notice. The combined Fermi/GBM+NITRATES 90% credible area is 245 deg2 and the 50% credible area is 63 deg2.

A plot of the probability skymap can be viewed here:

[skymap_plot](https://guano.swift.psu.edu/trigger_report?id=753338168/#:~:text=Probability%20Skymap)

The probability skymap file can be downloaded from the link here

[skymap_fits_file](https://guano.swift.psu.edu/files/753338168/0_n_PROBMAP)

Instructions on how to read and manipulate this map can be found here:

https://guano.swift.psu.edu/documentation

More details about this burst can be found on the trigger report page here:

https://guano.swift.psu.edu/trigger_report?id=753338168

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/

GCN Circular 38257

Subject
GRB 241115C: Fermi GBM Observation
Date
2024-11-16T21:50:57Z (6 months ago)
From
Lorenzo Scotton at UAH <lscottongcn@outlook.com>
Via
Web form
L. Scotton (UAH), S. Dalessi (UAH) and C. Meegan (UAH) report on behalf of
the Fermi Gamma-ray Burst Monitor Team:

"At 04:35:33.96 UT on 15 November 2024, the Fermi Gamma-ray Burst Monitor (GBM)
triggered and located GRB 241115C (trigger 753338138/241115191).
which was also detected by Swift/BAT-GUANO (S. Ronchini et al. 2024, GCN 38245).

The on-ground calculated location, using the Fermi GBM trigger data,
is RA = 257.26, Dec = 16.20 (J2000 degrees, equivalent to J2000 17h 9m, +16d 11'),
with a statistical uncertainty of 4.91 degrees. The Fermi GBM on-ground location 
is consistent with the Swift/BAT-NITRATES position.

The angle from the Fermi LAT boresight is 66 degrees.

The GBM light curve consists of a single emission episode with a duration (T90)
of about 5.1 s (50-300 keV). The time-averaged spectrum
from T0-1.0 to T0+7.0 s is best fit by
a power law function with an exponential high-energy cutoff.
The power law index is -1.77 +/- 0.08 and the cutoff energy,
parameterized as Epeak, is 53 +/- 7 keV.

The event fluence (10-1000 keV) in this time interval is
(2.1 +/- 0.1)E-06 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+0.32 s in the 10-1000 keV band is 9.9 +/- 0.4 ph/s/cm^2.

A Band function fits the spectrum equally well with
Epeak = 51 +/- 7 keV, alpha = -1.72 +/- 0.11 and beta = -2.61 +/- 0.49.

The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog:
https://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html

For Fermi GBM data and info, please visit the official Fermi GBM Support Page:
https://fermi.gsfc.nasa.gov/ssc/data/access/gbm/"

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