{
  "bibcode": "2025GCN.39892....1B",
  "eventId": "GRB 250327A",
  "createdOn": 1743120459909,
  "submittedHow": "email",
  "submitter": "Phil Evans at U of Leicester <pae9@star.le.ac.uk>",
  "body": "D.N. Burrows (PSU), M. A. Williams (PSU), S. Dichiara (PSU), J.P.\nOsborne (U. Leicester), K.L. Page (U. Leicester), V. D'Elia (SSDC &\nINAF-OAR), B. Sbarufatti (INAF-OAB), C. Salvaggio (INAF-OAB) and P.A.\nEvans report on behalf of the Swift-XRT team:\n\nWe have analysed 8.0 ks of XRT data for GRB 250327A, from 12.1 ks to\n47.5 ks after the  BAT trigger. The data are entirely in Photon\nCounting (PC) mode. The refined XRT position is RA, Dec = 248.1950,\n+61.6164 which is equivalent to:\n\nRA (J2000): 16 32 46.80\nDec(J2000): +61 36 58.9\n\nwith an uncertainty of 3.6 arcsec (radius, 90% confidence).\n\nThe light curve can be modelled with a power-law decay with a decay\nindex of alpha=0.92 (+0.22, -0.21).\n\nA spectrum formed from the PC mode data can be fitted with an absorbed\npower-law with a photon spectral index of 2.38 (+0.32, -0.29). The\nbest-fitting absorption column is  3.0 (+1.1, -1.0) x 10^21 cm^-2, in\nexcess of the Galactic value of 2.6 x 10^20 cm^-2 (Willingale et al.\n2013). The counts to observed (unabsorbed) 0.3-10 keV flux conversion\nfactor deduced from this spectrum  is 3.1 x 10^-11 (5.7 x 10^-11) erg\ncm^-2 count^-1. \n\nA summary of the PC-mode spectrum is thus:\nTotal column:\t     3.0 (+1.1, -1.0) x 10^21 cm^-2\nGalactic foreground: 2.6 x 10^20 cm^-2\nExcess significance: 4.6 sigma\nPhoton index:\t     2.38 (+0.32, -0.29)\n\nIf the light curve continues to decay with a power-law decay index of\n0.92, the count rate at T+24 hours will be 0.016 count s^-1,\ncorresponding to an observed (unabsorbed) 0.3-10 keV flux of 5.1 x\n10^-13 (9.3 x 10^-13) erg cm^-2 s^-1.\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/01299088.\n\nThis circular is an official product of the Swift-XRT team.\n",
  "circularId": 39892,
  "subject": "GRB 250327A: Swift-XRT refined Analysis"
}