List of Gamma Ray Bursts observed by the RHESSI satellite in the year 2010

The list includes major GRBs, that were not observed by RHESSI. If possible, the reason for not seeing it is given.
T90
T90 is the length of the time intervall, in which 90 per cent of all GRB counts in the 25-1500 keV-band are observed.
counts
total number of counts in the 25-1500 keV-band (after background subtraction)
signal/noise
significance of the GRB signal in the 25-1500 keV-band during the T90 time interval
polar angle
angle between RHESSI's rotation axis and the GRB direction, i.e. angle between Sun direction and GRB direction
reference
mostly GCN messages and Konus triggers. In a few cases, the reference is 'priv. comm. K. Hurley', i.e. private communication by Kevin Hurley. He maintains a master burst list of cosmic, SGR, and solar events (see e.g. IPN3 )
date start time
(UTC)		 reference peak time
(UTC) 		duration
(T90)
[sec]		 counts signal/
noise		 lightcurve direction
RA, Dec
[deg]		 polar
angle
[deg]		 comment
2010-02-11 10:33:23.30 Fermi 287577217, Konus 3278 10:33:46.55 28.80 2427 9.8 PNG / PS 120.933, 31.767 157.2  
2010-02-05 11:45:32.30 GCN 10397 (Fermi GBM) 11:45:52.55 7.20 509 4.5 PNG / PS 133.9, -23.0 140.8  
2010-01-19 18:25:10.30 GCN 10351 (Swift) 18:25:28.45 18.00 2598 12.7 PNG / PS 299.3, -53.1 33.0  
2010-01-18 02:23:29.60 Konus 3268, SPI ACS 11795, Suzaku 1431 02:23:34.50 5.40 774 7.0 PNG / PS      
2010-01-16 21:32:24.40 GCN 10333 (Fermi LAT) 21:32:35.10 14.60 2963 14.1 PNG / PS 305.0, 14.4 35.8  
2010-01-02 08:12:18.00 Konus 3263 08:12:49.50 57.00 7273 16.4 PNG / PS     decimation corrected

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