GCN Circular 32030

P. Veres and C. Meegan (both UAH)
report on behalf of the Fermi GBM Team:

"At 13:41:56.87 UT on 11 May 2022, the Fermi Gamma-Ray Burst Monitor (GBM)
triggered and located GRB 220511A (trigger 673969321 / 220511571)
which was also detected by Swift/BAT-GUANO (DeLaunay et al., GCN 32023
Not found
 
 
).
The Fermi GBM Final Real-time Localization (GCN 32018
Not found
 
 
) is consistent
with the Swift position.


The angle from the Fermi LAT boresight at the GBM trigger time is 112 degrees.

The GBM light curve consists of a single FRED-like pulse
with a duration (T90) of about 4.2 s (50-300 keV).
The time-averaged spectrum from T0 to T0+5.7 s is best fit by
a power law function with an exponential
high-energy cutoff.  The power law index is -0.85 +/- 0.05 and
the cutoff energy, parameterized as Epeak, is 199 +/- 11 keV.

The event fluence (10-1000 keV) in this time interval is
(7.62 +/- 0.23)E-6 erg/cm^2. The 1-sec peak photon flux measured
starting from T0+0.58 s in the 10-1000 keV band
is 20.3 +/- 0.5 ph/s/cm^2.

A Band function fits the spectrum equally well
with Epeak= 155 +/- 14 keV, alpha = -0.70 +/- 0.08 and beta = 2.18 +/- 0.12.

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/"