TITLE: GCN CIRCULAR NUMBER: 14553 SUBJECT: Swift-XRT X-ray afterglow candidate for GRB 130504A (BAT trigger 555096) DATE: 13/05/04 09:28:24 GMT FROM: Phil Evans at U of Leicester P. D'Avanzo (INAF-OAB), A. Melandri (INAF-OAB), K.L. Page (U. Leicester), P.A. Evans (U. Leicester) report on behalf of the Swift-XRT team: We have analysed 654 s of XRT data for GRB 130504A, from 99 s to 754 s after the BAT trigger. The data are entirely in Photon Counting (PC) mode. No X-ray afterglow is detected within the BAT error circle (Cummings et al. GCN 14551). We note however the presence of a bright, uncatalogued, fading X-ray source at the following refined position RA, Dec = 272.45484, -16.31423 which is equivalent to: RA (J2000): 18 09 49.16 Dec(J2000): -16 18 51.2 with an uncertainty of 3.5 arcsec (radius, 90% confidence). This position is about 5.5 arc min away from the BAT position. Given its fading nature, we propose it as the X-ray afterglow of GRB 130504A. The light curve can be modelled with a power-law decay with a decay index of alpha=0.79 (+/-0.19). A spectrum formed from the PC mode data can be fitted with an absorbed power-law with a photon spectral index of 1.7 (+/-0.4). The best-fitting absorption column is 1.6 (+0.5, -0.4) x 10^22 cm^-2, in excess of the Galactic value of 8.1 x 10^21 cm^-2 (Kalberla et al. 2005). The counts to observed (unabsorbed) 0.3-10 keV flux conversion factor deduced from this spectrum is 7.4 x 10^-11 (1.3 x 10^-10) erg cm^-2 count^-1. A summary of the PC-mode spectrum is thus: Total column: 1.6 (+0.5, -0.4) x 10^22 cm^-2 Galactic foreground: 8.1 x 10^21 cm^-2 Excess significance: 2.8 sigma Photon index: 1.7 (+/-0.4) If the light curve continues to decay with a power-law decay index of 0.79, the count rate at T+24 hours will be 0.021 count s^-1, corresponding to an observed (unabsorbed) 0.3-10 keV flux of 1.5 x 10^-12 (2.8 x 10^-12) erg cm^-2 s^-1. The results of the XRT-team automatic analysis are available at http://www.swift.ac.uk/xrt_products/00555096. This circular is an official product of the Swift-XRT team.