[vsnet-grb-info 2885] GRB 060206: Swift/UVOT Observations
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Fri Feb 10 07:30:40 JST 2006
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 4722
SUBJECT: GRB 060206: Swift/UVOT Observations
DATE: 06/02/09 22:27:58 GMT
FROM: Padi Boyd at GSFC <padi at milkyway.gsfc.nasa.gov>
P. Boyd (GSFC), D. Morris (PSU), F. Marshall (GSFC), N. Gehrels (GSFC)
on behalf of the Swift/UVOT team report:
The Swift/UVOT began observing the bright afterglow of GRB 060206 at
04:47:52 UT on 2006-02-06, approximately 57s after the BAT trigger (Morris
et al., GCN 4682). The afterglow is well detected in the individual B and
V exposures during the initial observation. The afterglow re-brightens in
both filters between 2000 to 5000-s after the BAT trigger. After this
event, the flux decays in both filters with a slope of ~1.15.
Filter T_range(s) Exp(s) Average mag
V 57-36588 2618 18.8
B 1662-34946 2911 21.3
Reported times are in seconds since BAT trigger.
In a follow-up observation, beginning about 0.8 d after the BAT trigger,
the source is not detected in B nor V down to the following 3-sigma
magnitude upper limits:
Filter T_range(s) Exp(s) mag upper limit
V 69308-150688 5001 >21.7
B 69656-150353 4679 >22.6
The afterglow is not detected in any other UVOT filter down to the
following 3-sigma magnitude upper limits:
Filter T_range(s) Exp(s) mag
U 1637-23385 1161 >21.5
UVW1 1757-5619 256 >20.6
UVM2 1733-30466 514 >21.3
UVW2 1686-35861 2638 >22.7
These magnitudes are uncorrected for Galactic extinction;
E(B-V) = 0.013.
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