TITLE: GCN CIRCULAR NUMBER: 38570 SUBJECT: GRB 241213B: Swift-XRT observations DATE: 24/12/14 17:30:10 GMT FROM: Phil Evans at U of Leicester pae9@star.le.ac.uk
A.P. Beardmore (U. Leicester), M. Capalbi (INAF-IASFPA), M. Perri (SSDC & INAF-OAR), V. D'Elia (SSDC & INAF-OAR), J.A. Kennea (PSU), D.N. Burrows (PSU), M. A. Williams (PSU), J.P. Osborne (U. Leicester) and P.A. Evans (U. Leicester) reports on behalf of the Swift-XRT team:
Swift-XRT has performed follow-up observations of the MAXI-detected burst GRB 241213B in a series of observations tiled on the sky. The total exposure time is 2.2 ks, distributed over 7 tiles; the maximum exposure at a single sky location in the tiling was 822 s. The data were collected between T0+54.1 ks and T0+60.2 ks, and are entirely in Photon Counting (PC) mode.
One uncatalogued X-ray source has been detected, it is below the RASS limit and shows no definitive signs of fading. Therefore, at the present time we cannot confirm this as the afterglow. Details of this source are given below:
Source 1: RA (J2000.0): 331.7177 = 22:06:52.25 Dec (J2000.0): +4.0971 = +04:05:49.6 Error: 9.0 arcsec (radius, 90% conf.) Count-rate: 0.0185 [+0.0089, -0.0068] ct s^-1 Distance: 1169 arcsec from MAXI position. Flux: (1.21 [+0.59, -0.44])e-9 erg cm^-2 s^-1 (observed, 0.3-10 keV)
The results of the XRT-team automatic analysis of the tiled XRT observations, including a position-specific upper limit calculator, are available at https://www.swift.ac.uk/xrt_products/TILED_GRB00130.
This circular is an official product of the Swift-XRT team.
View this GCN Circular online at https://gcn.nasa.gov/circulars/38570. --- To unsubscribe, open this link in a web browser: https://gcn.nasa.gov/unsubscribe/eyJhbGciOiJIUzI1NiJ9.eyJlbWFpbCI6InZzbmV0LW...