GCN Circular 12874
David Gruber (MPE) reports on behalf of the Fermi GBM Team: "At 04:04:25.06 UT on 19 January 2012, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 120119A (trigger 348638667 / 120119170). which was also detected by the Swift/BAT and Swift/XRT (Beardmore et al. 2012, GCN 12859) The GBM on-ground location is consistent with the Swift position. The angle from the Fermi LAT boresight is 31.4 degrees. This burst was also independently detected by INTEGRAL SPI-ACS. The GBM light curve shows several overlapping pulses with a duration (T90) of about 55 s (50-300 keV). The time-averaged spectrum from T0-1.5 s to T0+53.8 s is best fit by a Band function with Epeak = 189.2 +/- 8.3 keV, alpha = -0.98 +/- 0.03, and beta = -2.36 +/- 0.09. The event fluence (10-1000 keV) in this time interval is (3.87 +/- 0.01)E-05 erg/cm^2. The 1-sec peak photon flux measured starting from T0+14.5 s in the 10-1000 keV band is 16.86 +/- 0.39 ph/s/cm^2. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog."