GCN Circular 7808
Subject
GRB 080603B: Swift/UVOT detection of the afterglow
Date
2008-06-04T13:57:29Z (16 years ago)
From
Paul Kuin at MSSL <npkuin@googlemail.com>
N. P. M. Kuin (MSSL/UCL), and V. Mangano (INAF-IASFPA), report on behalf
of the Swift UVOT team
The Swift UltraViolet/Optical Telescope (UVOT) began observations
of GRB 080603A, on June 3, 2008, at 19:39:07 UT, 63 seconds after
the initial Swift BAT trigger (Mangano et al., GCN Circ. 7794)..
The refined uvot position is
RA = 11:46:07.66 = 176.5316
DEC =+68:03:39.99 = 68.061105
with an error or 0.3".
The first finding chart in the wh filter has problems due to the
brightness of the image, and needs detailed analysis. We start
our report with the second finding chart.
The magnitudes with 1-sigma errors for GRB080603B are given below
for the initial observation sequence.
Filter Tstart(s) Tstop(s) Exp(s) Magnitude
v 187.8 393.1 202 16.48 +/- 0.06
uvm2 5778.0 5977.8 197 > 19.51 (3-sigma UL)
uvw1 5983.9 6183.7 197 20.02 +/- 0.56
u 6188.8 6388.6 197 18.80 +/- 0.23
b 6395.3 12274.3 643 19.34 +/- 0.14
The absence of a detection in the uvm2 filter is consitent with
the reported redshift of 2.69 (Fynbo et al., GCN Circ. 7797).
Magnitude variation in the b observations shor evidence
of flaring or rebrightening..
The values quoted above are on the UVOT Photometric System
(Poole et al, 2008, MNRAS 383,627). They are not corrected for the
expected galactic reddening of E(B-V) = 0.013 in the direction of
the burst (Schlegel et al. 1998).