[vsnet-grb-info 9870] GRB 101011A: Swift/UVOT observations
GCN Circulars
gcncirc at capella2.gsfc.nasa.gov
Tue Oct 12 23:08:57 JST 2010
TITLE: GCN CIRCULAR
NUMBER: 11338
SUBJECT: GRB 101011A: Swift/UVOT observations
DATE: 10/10/12 14:08:49 GMT
FROM: Massimiliano de Pasquale at MSSL-UCL <mdp at mssl.ucl.ac.uk>
M. De Pasquale (MSSL-UCL) and J. Cannizzo (GSFC)
report on behalf of the Swift/UVOT team:
The Swift/UVOT began settled observations of the field of GRB 101011A
85s after the BAT trigger (Cannizzo et al., GCN Circ. 11331).
Summing up white band exposures up to 1374s after the trigger, including
the finding chart, we find a strong indication (2.9 sigma level) of an
uncatalogued source at
RA = 03h 13m 10.77s, Dec = -65d 58m 54.0s (J2000)
RA = 48.29487, Dec = -65.98167 (J2000)
with an error of 1.1 arcseconds. This refined position is within 0.5
arcseconds from the XRT refined position (Evans et al., GCN Circ. 11333)
and supersedes the previous onegiven in Holland et al. (GCN Circ. 11334).
In the individual and summed UVOT exposures in other filters, no optical
afterglow is detected. Preliminary 3-sigma upper limits using the UVOT
photometric system (Poole et al. 2008, MNRAS, 383, 627) for the first
finding chart (FC) exposure and subsequent exposures are:
Filter T_start(s) T_stop(s) Exp(s) Mag
white(FC) 85 235 147 >21.3
white 85 1374 373 21.7 ± 0 0.4
white 4311 6627 393 >22
v 627 18725 1375 >20.8
b 533 41918 1055 >21.4
u 297 41737 2865 >22.0
uw1 577 47696 2595 >21.7
um2 652 46017 2996 >21.7
uw2 603 17812 376 >21.5
The values quoted above are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.03 in the direction of the burst
(Schlegel et al. 1998).
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