GRB 101130A, GRB 101130

S. Golenetskii, R.Aptekar, D. Frederiks, E. Mazets, V. Pal'shin,
P. Oleynik, M. Ulanov, D. Svinkin, and T. Cline on behalf
of the Konus-Wind team, report:

GRB 101130A (localized by IPN: Hurley et al., GCN 11437
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triggered Konus-Wind at T0=34766.178s UT (09:39:26.178)

The burst light curve starts with a short (~1.5 s) pulse,
followed by a weaker pulse at ~T0+55 s (with a duration of ~6 s).
The emission is seen up to ~1 MeV.
The Konus-Wind light curve of this GRB is available at
http://www.ioffe.ru/LEA/GRBs/GRB101130_T34766/

As observed by Konus-Wind the burst
had a fluence of 3.1(+1.1/-1.0)x10-6 erg/cm2,
and a 16-ms peak flux measured from T0-0.048s
of 2.8(+0.8/-0.7)x10-6 erg/cm2/s
(both in the 20 keV - 1 MeV energy range).

The time-integrated spectrum of the burst
(from T0 to T0+65.792 s) is best fit
in the 20 keV - 1 MeV range by a simple power law model
with the index = -1.85 (-0.3, +0.35), chi2 = 44/48 dof.

The spectrum of the initial short pulse
(measured from T0 to T0+0.256 s) is best fit
in the 20 keV - 1 MeV range by a power law
with exponential cutoff model, for which
alpha = -0.6 (-0.6, +0.9),
and Ep = 190(-55, +135) keV, chi2 = 26/18 dof.

The spectrum of the second pulse
(measured from T0+57.600 to T0+65.792 s) is best fit
in the 20 keV - 1 MeV range by a simple power law model
with the index = -2.1 (-0.5, +0.7), chi2 = 49/48 dof.


All the quoted results are preliminary.
All the quoted errors are at the 90% confidence level

K. Hurley, on behalf of the MESSENGER and Odyssey GRB teams,

S. Golenetskii, R. Aptekar, E. Mazets, V. Pal'shin, D. Frederiks, and
T. Cline on behalf of the Konus-Wind team,

J. Goldsten, on behalf of the MESSENGER NS GRB team, 

I. G. Mitrofanov, D. Golovin, M. L. Litvak, and A. B. Sanin,
on behalf of the HEND-Odyssey GRB team,  and

W. Boynton, C. Fellows, K. Harshman, H. Enos, and R. Starr, on
behalf of the GRS-Odyssey GRB team, report:

Konus-Wind, MESSENGER GRNS, and Mars Odyssey HEND observed this
burst at 34766 s on November 30, 2010.  As seen by Konus-Wind, the 
time history displayed a short (~1.5 s long) pulse, and a weak 
pulse at ~T0+50 s (with a duration of ~6 s). There is evidence
for this second pulse in the MESSENGER data at the same time after 
the main pulse, confirming their common origin.

We have localized it to a preliminary, 3 sigma error box whose 
coordinates are

	         RA(2000)			  Dec(2000)
CENTER:     61.803o=04 h 07 m 12.73 s    -16.759o=-16 o 45 '  33.09 "
CORNERS:    62.468o=04 h 09 m 52.39 s    -17.210o=-17 o 12 '  34.62 "   
            62.953o=04 h 11 m 48.62 s    -17.213o=-17 o 12 '  45.80 "      
            60.654o=04 h 02 m 37.06 s    -16.270o=-16 o 16 '  11.27 "    
            61.144o=04 h 04 m 34.57 s    -16.297o=-16 o 17 '  48.56 "

The error box area is ~1500 sq. arcmin.  This error box may be improved.
Time history and spectral information will be reported in a forthcoming
GCN Circular.