TITLE: GCN CIRCULAR NUMBER: 27497 SUBJECT: GRB 200405B: Swift/BAT-GUANO detection and *possible* arcminute localization of a short GRB DATE: 20/04/05 22:52:50 GMT FROM: Aaron Tohuvavohu at U Toronto James DeLaunay (PSU), Aaron Tohuvavohu (U Toronto), and Jamie Kennea (PSU) report: Swift/BAT did not trigger on GRB 200405B (T0: 2020-04-05 03:53:38 UTC). The INTEGRAL/SPI-ACS Notice #8579, distributed at T0+35 seconds triggered the Swift Mission Operations Center operated Gamma-ray Urgent Archiver for Novel Opportunities (GUANO; Tohuvavohu et al. 2020, in prep). Upon trigger by these notices, GUANO sent a command to the Swift Burst Alert Telescope (BAT) to save 90 seconds of BAT event-mode data from [-45,+45] seconds around the time of the burst. All the requested event mode data was delivered to the ground. In a ground analysis of the data, we detect the burst in the full detector-summed rates (no localization information) with an SNR of ~9. The detected duration is ~0.5 seconds. With a maximum likelihood analysis (DeLaunay et al. 2020, in prep.) on the event-mode data we detect a location for the burst with a square root of the test statistic, sqrt(TS), of 12.4. The sqrt(TS) behaves similarly to SNR. Using the normal BAT imaging technique, we find an SNR of ~4 at the same location. The BAT ground-calculated position is RA, Dec = 62.7894, -51.5326 deg which is RA(J2000) = 4h 11m 9.5s Dec(J2000) = -51d 31’ 57.4” with an uncertainty of 4 arcmin, (radius, sys+stat, 90% containment). The partial coding was 11.6%. Due to the low partial coding, and the lack of any localization information from SPI-ACS for a consistency check, we stress that while this localization is significant, we cannot be certain of whether or not the burst actually originated from outside the BAT coded field-of-view. XRT and UVOT follow-up has been triggered and observations of this region have already begun. Results of follow-up observations will be reported in future circulars. GUANO is a fully autonomous, extremely low latency, spacecraft commanding pipeline designed for targeted recovery of BAT event mode data around the times of compelling astrophysical events to enable more sensitive GRB searches. A live reporting of Swift/BAT event data recovered by GUANO can be found at: https://www.swift.psu.edu/guano/