{
  "bibcode": "2021GCN.29495....1T",
  "body": "A. Tohuvavohu (U. Toronto), B. Sbarufatti (PSU), D.N. Burrows (PSU),\nK.L. Page (U. Leicester), A.P. Beardmore (U. Leicester), P.A. Evans (U.\nLeicester), A. Melandri (INAF-OAB), T. Sbarrato (INAF-OAB), P. D'Avanzo\n(INAF-OAB) and E. Troja report on behalf of the Swift-XRT team:\n\nWe have analysed 6.8 ks of XRT data for GRB 210212A (Troja et al. GCN\nCirc. 29487), from 109 s to 34.2 ks after the  BAT trigger. The data\ncomprise 337 s in Windowed Timing (WT) mode with the remainder in\nPhoton Counting (PC) mode. The enhanced XRT position for this burst was\ngiven by Beardmore et al. (GCN Circ. 29489).\n\nThe light curve can be modelled with an initial power-law decay with an\nindex of alpha=2.27 (+0.28, -0.50), followed by a break at T+194 s to\nan alpha of 3.79 (+0.28, -0.23).\n\nA spectrum formed from the WT mode data can be fitted with an absorbed\npower-law with a photon spectral index\tof 1.55 (+0.13, -0.12). The\nbest-fitting absorption column is  1.6 (+0.6, -0.4) x 10^21 cm^-2,\nconsistent with the Galactic value of 1.1 x 10^21 cm^-2 (Willingale et\nal. 2013). The counts to observed (unabsorbed) 0.3-10 keV flux\nconversion factor deduced from this spectrum  is 4.4 x 10^-11 (5.0 x\n10^-11) erg cm^-2 count^-1. \n\nA summary of the WT-mode spectrum is thus:\nTotal column:\t     1.6 (+0.6, -0.4) x 10^21 cm^-2\nGalactic foreground: 1.1 x 10^21 cm^-2\nExcess significance: <1.6 sigma\nPhoton index:\t     1.55 (+0.13, -0.12)\n\nIf the light curve continues to decay with a power-law decay index of\n3.79, the count rate at T+24 hours will be 5.3 x 10^-10 count s^-1,\ncorresponding to an observed (unabsorbed) 0.3-10 keV flux of 2.3 x\n10^-20 (2.6 x 10^-20) erg cm^-2 s^-1.\n\nThe results of the XRT-team automatic analysis are available at\nhttp://www.swift.ac.uk/xrt_products/01032183.\n\nThis circular is an official product of the Swift-XRT team.",
  "circularId": 29495,
  "createdOn": 1613146696000,
  "email": "pae9@leicester.ac.uk",
  "subject": "GRB 210212A: Swift-XRT refined Analysis",
  "submitter": "Phil Evans at U of Leicester  <pae9@leicester.ac.uk>",
  "eventId": "GRB 210212A"
}