TITLE: GCN CIRCULAR NUMBER: 27500 SUBJECT: GRB 200405B: Swift-XRT observations DATE: 20/04/06 15:18:06 GMT FROM: Andy Beardmore at U Leicester B. Sbarufatti (PSU), D.N. Burrows (PSU), J. D. Gropp (PSU), K.L. Page (U. Leicester), A.P. Beardmore (U. Leicester), A. Melandri (INAF-OAB), T. Sbarrato (INAF-OAB), P. D'Avanzo (INAF-OAB) and P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team: Swift-XRT has performed follow-up observations of the INTEGRAL/SPI-ACS and Swift-BAT GUANO detected possible short burst GRB 200405B (James DeLaunay et al. GCN Circ. 27497), collecting 5.0 ks of Photon Counting (PC) mode data between T0+66.6 ks and T0+80.0 ks. Four uncatalogued X-ray sources have been detected, however none of them is above the RASS limit or shows definitive signs of fading. Therefore, at the present time we cannot identify which, if any, is the afterglow. We note that Source 2 lies within the 4 arcmin BAT error region reported in GCN Circ. 27497. Details of these sources are given below: Source 1: RA (J2000.0): 62.6009 = 04:10:24.21 Dec (J2000.0): -51.4435 = -51:26:36.5 Error: 5.5 arcsec (radius, 90% conf.) Count-rate: (1.87 [+0.90, -0.69])e-3 ct s^-1 Distance: 530 arcsec from BAT position. Flux: (1.15 [+0.55, -0.43])e-13 erg cm^-2 s^-1 (observed, 0.3-10 keV) Source 2: RA (J2000.0): 62.8248 = 04:11:17.95 Dec (J2000.0): -51.5687 = -51:34:07.5 Error: 6.5 arcsec (radius, 90% conf. [Enhanced position]) Count-rate: (3.31 [+1.13, -0.93])e-3 ct s^-1 Distance: 152 arcsec from BAT position. Flux: (4.1 [+1.4, -1.1])e-13 erg cm^-2 s^-1 (observed, 0.3-10 keV) Source 3: RA (J2000.0): 62.5137 = 04:10:3.28 Dec (J2000.0): -51.4509 = -51:27:03.3 Error: 4.6 arcsec (radius, 90% conf.) Count-rate: (1.96 [+0.97, -0.73])e-3 ct s^-1 Distance: 684 arcsec from BAT position. Source 4: RA (J2000.0): 62.6146 = 04:10:27.49 Dec (J2000.0): -51.5329 = -51:31:58.3 Error: 4.3 arcsec (radius, 90% conf.) Count-rate: (3.74 [+1.18, -0.99])e-3 ct s^-1 Distance: 391 arcsec from BAT position. Flux: (1.20 [+0.38, -0.32])e-13 erg cm^-2 s^-1 (observed, 0.3-10 keV) The results of the XRT-team automatic analysis of the XRT observations, including a position-specific upper limit calculator, are available at https://www.swift.ac.uk/ToO_GRBs/00020979. This circular is an official product of the Swift-XRT team.