[vsnet-grb-info 13405] Swift/UVOT observations of GRB130603A
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Jun 4 04:37:42 JST 2013
TITLE: GCN CIRCULAR
NUMBER: 14738
SUBJECT: Swift/UVOT observations of GRB130603A
DATE: 13/06/03 19:36:24 GMT
FROM: Massimiliano de Pasquale at MSSL-UCL <m.depasquale at ucl.ac.uk>
M. De Pasquale (MSSL/UCL) and A. Melandri (INAF/OAB) report on behalf
of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 130603A
3325 s after the BAT trigger (Melandri et al., GCN Circ. 14731). The
uncatalogued source reported in Melandri et al., GCN Circ. 14732, is
detected in the summed exposures.
Preliminary detections and 3-sigma upper limits using the UVOT
photometric system (Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for
the summed exposures are:
Filter T_start(s) T_stop(s) Exp(s) Mag
white 3686 5322 393 19.61 ± 0.15
v 4097 5562 197 >19.02
b 3481 16641 1278 19.71 ± 0.15
u 3275 15729 1278 19.19 ± 0.13
uvw1 4507 4707 197 19.62 ± 0.39 (2.8 sigma)
uvm2 4302 4502 197 >19.63
uvw2 3892 5528 393 20.25 ± 0.37 (2.8 sigma)
The possible detection of the optical source in uw2 filter indicates
a redshift z < ~1.5 for this event.
The magnitudes in the table are not corrected for the Galactic
extinction due to the reddening of E(B-V) = 0.06 in the direction of
the burst (Schlegel et al. 1998).
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