TITLE: GCN CIRCULAR NUMBER: 25726 SUBJECT: Update to the Fermi GBM Localizations DATE: 19/09/11 13:28:39 GMT FROM: Adam Goldstein at Fermi-GBM, USRA The Fermi GBM Team reports an improvement to its automated final localizations for onboard triggered GRBs. These are the localizations reported in the "Fermi GBM Final Real-time Localization" GCN Circulars and the "GCN/FERMI_GBM_FINAL_POSITION" GCN Notices. The RoboBA, in operation since early 2016, has been improved to provide more accurate localizations, and the systematic uncertainty has been reduced. Specifically, the overall estimated systematic uncertainty for localizations is a mixture of two Gaussians, one with a radius of 1.8 degrees (52% contribution) and one with a radius of 4.1 degrees (47% contribution). The RoboBA provides an estimate on the classification of the GRB: long or short, with an accuracy of 92-95% relative to the T90 = 2 s split. Based on the RoboBA classification, a long GRB will have a systematic uncertainty of 1.9 degrees (58% contribution) and 4.1 degrees (42% contribution). A short GRB will have a systematic uncertainty of 2.6 degrees (39% contribution) and 4.4 degrees (61% contribution). The HEALPix FITS files provided for each localization will already incorporate the systematic. The median 50% localization area has been reduced from 81 square degrees to 46 square degrees, and the median 90% localization area has been reduced from 400 square degrees to 200 square degrees. The 5%-95% range of the 90% localization area has been reduced from (~400-6000) square degrees to (~170-1100) square degrees. We anticipate an automated localization for ~95% of triggered GRBs within 10 minutes of trigger time, and we will continue providing Human-in-the-Loop localizations for the rest of the triggered GRBs with a latency of up to a couple of hours. For more details on the RoboBA, systematics estimation, and localization improvement, please see https://arxiv.org/abs/1909.03006