NOTE: Possible detection in uu at T+44849.5
NOTE: Possible detection in vv at T+51723.1 sum

=========== Draft Upper Limit Circular ========

GRB 140716A: Swift/UVOT Upper Limits

L. M. Z. Hagen (PSU) and K. L. Page (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 140716A
34072 s after the BAT trigger (***Author*** et al., GCN Circ. ????).
No optical afterglow consistent with the optical position
(Knust et al. GCN Circ. 16601)
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 initial exposures are:

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

v                40559        57642         2081         >19.6
u                34072        56904         2151         >19.9

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.13 in the direction of the burst
(Schlegel et al. 1998).


=========== Draft Detection Circular ========

GRB 140716A: Swift/UVOT Detection

L. M. Z. Hagen (PSU) and K. L. Page (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 140716A
34072 s after the BAT trigger (***Author*** et al., GCN Circ. ????).
A source consistent with the optical position
(Knust et al. GCN Circ. 16601)
is detected in the initial UVOT exposures.

Preliminary detections 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

v                40559        57642         2081         20.20 +/- 0.23
u                34072        51148         1588         20.21 +/- 0.20

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.13 in the direction of the burst
(Schlegel et al. 1998).