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TITLE:   GCN CIRCULAR
NUMBER:  8107
SUBJECT: GLAST Burst Monitor detection of GRB080816
DATE:    08/08/19 12:09:51 GMT
FROM:    Andreas von Kienlin at MPE  <azk@mpe.mpg.de>

Andreas von Kienlin, Sheila McBreen and Elisabetta Bissaldi (MPE) 
report on behalf of the GLAST Burst Monitor Team: 

"At 12:04:18 UT on 2008 Aug 16, the GLAST Burst Monitor (GBM) 
triggered and located GRB 080816 (GBM 080816.503 / trigger 240581059). 
The on-ground calculated location, using the GBM trigger data, is 
RA = 156.9, Dec = +54.60 (J2000 degrees) 
(equivalent to J2000 10h 28m, +54d 36'), 
with an uncertainty of 2.3 degrees (radius, 1-sigma containment, statistical 
only; there is additionally a systematic error which is currently estimated 
to be 2 to 3 degrees). The angle from the Large Area Telescope (LAT) 
boresight is 55 degrees at ~T+35 sec. 

This GRB has a duration of approximately 70 s and contains 4 peaks. 
The preliminary averaged time spectrum in the 10 keV to 500 keV energy band
from T-1 to T+69 s is well fit by a power law function with an exponential 
high energy cutoff. The power law index is -0.57 +/-0.14 and the cutoff 
energy, parameterized as Epeak, is 146.7 +/-14.5 keV, with a reduced 
chi-square of 1.2 for 291 degrees of freedom. 

The fluence in the 50-300 keV band is (1.86 +/- 0.20) x 10^-5 erg/cm2. 
The 1-sec photon flux measured from T+35 sec in the 50-300 keV band 
is  3.48 +/-0.66  ph/cm2/sec. All the quoted errors are at the 90% 
confidence level.
These spectral analysis results presented above are preliminary; the final 
results will be published in the GBM GRB Catalog." 

////////////////////////////////////////////////////////////////////////
TITLE:   GCN CIRCULAR
NUMBER:  8111
SUBJECT: GLAST Burst Monitor detection of a GRB: 080816B
DATE:    08/08/21 22:31:00 GMT
FROM:    Rob Preece at UAH  <Rob.Preece@nasa.gov>

R. D. Preece (UAHuntsville) and A.J. van der Horst (NASA/ORAU) report  
on behalf of the GLAST Burst Monitor Team:

"At 23:44:01 UT on 16 August, 2008, the GLAST Burst Monitor (GBM)
triggered and located GRB 080816B (trigger 240623035 / 080816.989).
The on-ground calculated location, using the GBM trigger data, is
RA = 288.5, Dec = -6.5 (J2000 degrees)
(equivalent to J2000 19h 14m, -06d 30'),
with an uncertainty of 5.2 degrees (radius, 1-sigma containment,  
statistical only; there is additionally a systematic error which is  
currently estimated to be 2 to 3 degrees). The angle from the Large  
Area Telescope (LAT) boresight is 70 degrees.

This GRB was about 5 s long with 2 peaks, showing structure on the 64  
ms time scale. The time-averaged spectrum from T-3.584 to T+1.536 s,  
in the energy range 6 keV to 3500 keV, is best fit with a power law  
times exponential cutoff. The power law index is -0.37 +/- 0.17 and  
the cutoff energy, parameterized as Epeak, is 1230 +/- 230 keV. We  
note that this is a hard event. The average photon flux is 1.38 +/-  
0.08 ph/s-cm^2 in the energy interval 25 - 1000 keV.

The spectral analysis results presented above are preliminary;
final results will be published in the GBM GRB Catalog."