[vsnet-grb-info 13061] GRB 130327B: Swift/XRT source is not the afterglow
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Sat Apr 20 05:11:37 JST 2013
TITLE: GCN CIRCULAR
NUMBER: 14398
SUBJECT: GRB 130327B: Swift/XRT source is not the afterglow
DATE: 13/04/19 20:11:29 GMT
FROM: Hans Krimm at NASA-GSFC <hans.krimm at nasa.gov>
H. A. Krimm (CRESST/GSFC/USRA) and E. Troja (NASA/GSFC/CRESST) for the Swift team:
Swift carried out an additional 4.6 ksec observation of the field containing GRB
130327B (e.g. Longo et al, GCN 14344; Ohno et al, GCN 14347), starting at
2013-04-18 12:43:13 UT, approximately 22 days after the burst. The source
reported in Krimm & Mangano (GCN 14353) as a possible afterglow to GRB 130327B
is still detected at a rate of 0.002 ± 0.001 cts/s (0.3-10 keV), which is
statistically consistent with the rate reported in GCN 14353. Since we would
expect a GRB afterglow to have faded over this time period, we conclude that the
XRT source is not associated with GRB 130327B, and is instead a background
source, possibly an AGN.
No further Swift observations are planned.
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