[vsnet-grb-info 13236] Swift/UVOT observations of GRB130505A
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Mon May 6 01:28:44 JST 2013
TITLE: GCN CIRCULAR
NUMBER: 14573
SUBJECT: Swift/UVOT observations of GRB130505A
DATE: 13/05/05 16:28:36 GMT
FROM: Massimiliano de Pasquale at MSSL-UCL <m.depasquale at ucl.ac.uk>
M. De Pasquale (MSSL/UCL) and J. K. Cannizzo (NASA/UMBC) report on behalf
of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 130505A
107 s after the BAT trigger (Cannizzo et al., GCN Circ. 14563). A bright
but
rapidly fading source is detected in the finding chart and initial exposures
within the XRT error circle (Evans et al., GCN Circ. 14569).
The preliminary UVOT position is:
RA(J2000) = 09:08:14.64 = 137.0610
DEC(J2000) = +17:29:05.2 = +17.48478
with a 90%-confidence error radius of about 0.5 arc sec.
Preliminary detections and 3-sigma upper limits using the UVOT
photometric system (Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for
the early exposures are:
Filter T_start(s) T_stop(s) Exp(s) Mag
white (FC) 107 256 147 14.14 ± 0.05
white 3952 4151 197 17.96 ± 0.07
v 4362 4561 197 17.50 ± 0.11
b 3503 3946 197 17.71 ± 0.08
u 320 542 218 14.66 ± 0.04
uvw1 4772 4971 197 19.28 ± 0.29 (~3
sigma)
uvm2 4567 4766 197 >19.6
uvw2 4158 4357 197 >19.9
The non-detection of the optical source in um2 and uw2 filters is
consistent with the redshift z=2.27 found by Tanvir et al (GCN Circ. 14567)
The magnitudes in the table are not corrected for the Galactic
extinction due to the reddening of E(B-V) = 0.04 in the direction of
the burst (Schlegel et al. 1998).
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