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GCN Circular 26277

Subject
GRB 191122A: Swift/UVOT Upper Limits
Date
2019-11-23T01:05:16Z (5 years ago)
From
Paul Kuin at MSSL <npkuin@gmail.com>
N. P. M. Kuin (UCL-MSSL) and B. Sbarufatti (PSU)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 191122A
104 s after the BAT trigger (Sbarufatti et al., GCN Circ. 26269).
No optical afterglow consistent with the XRT position
(Evans GCN Circ. 26270,26272)
is detected in the initial UVOT exposures.
Preliminary 3-sigma upper limits using the UVOT photometric system
(Breeveld et al. 2011, AIP Conf. Proc. 1358, 373) for the first
finding chart (FC) exposure and subsequent exposures are:

Filter         T_start(s)   T_stop(s)      Exp(s)         Mag

white_FC           104          253          147         >21.1
u_FC               316          566          246         >20.4
white              104        11801         1305         >22.0
v                  647         6097          432         >20.2
b                  572        10938         1121         >21.9
u                  316         6696          642         >20.5
w1                 696         6508          413         >20.1
m2                 846         6303          413         >21.2
w2                 797         5893          413         >20.1

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.01 in the direction of the burst
(Schlegel et al. 1998).
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