TITLE: GCN CIRCULAR NUMBER: 11341 SUBJECT: GRB 101014A: Fermi GBM detection DATE: 10/10/14 19:12:34 GMT FROM: David Tierney at UCD Dave Tierney (UCD) and Adam Goldstein (UAH) report on behalf of the Fermi GBM Team: "At 04:11:52.62 UT on 14 October 2010, the Fermi Gamma-Ray Burst Monitor triggered and located GRB 101014A (trigger 308722314 / 101014175 ). The on-ground calculated location, using the GBM trigger data, is RA = 26.94, DEC = -51.07 (J2000 degrees, equivalent to 01 h 47 m, -51 d 04 '), with an uncertainty of 1.0 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 Fermi LAT boresight is 54 degrees. This burst resulted in a Fermi spacecraft repointing maneuver. This burst was also independently detected by INTEGRAL SPI-ACS. The GBM light curve consists of multiple pulses with a T90 of about 450 s (50-300 keV). The time-averaged spectrum from T0+1.5 s to T0+473.6 s is best fit by a Band function with Epeak = 181.40 (+5.66/-5.44) keV, alpha = -1.27 (+0.01/-0.01), and beta = -2.07 (+0.02/-0.02) (C-stat of 2499.1 for 591 d.o.f.). The event fluence (10-1000 keV) in this time interval is (2.072 +/- 0.009)E-04 erg/cm^2. The 1-sec peak photon flux measured starting from T0+208.77 s in the 8-1000 keV band is 58.96 +/- 0.42 ph/s/cm^2. The spectral analysis results presented above are preliminary; final results will be published in the GBM GRB Catalog."