NOTE: Possible detection in vv at T+78109.0
NOTE: Possible detection in w2 at T+77202.7
NOTE: Possible detection in m2 at T+79020.4

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

GRB 140809A: Swift/UVOT Upper Limits

***UBS*** (***INSTITUTION***) and ***BA*** (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 140809A
77203 s after the GBM trigger (***Author*** et al., GCN Circ. ????).
No optical afterglow consistent with the optical position
(Masi GCN Circ. 16675)
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                78109        79016          885         >17.7
m2               79020        79197          174         >18.9
w2               77203        78103          886         >19.7

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).


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

GRB 140809A: Swift/UVOT Detection

***UBS*** (***INSTITUTION***) and ***BA*** (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 140809A
77203 s after the GBM trigger (***Author*** et al., GCN Circ. ????).
A source consistent with the optical position
(Masi GCN Circ. 16675)
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                78109        78409          295         17.80 +/- 0.07
m2               79020        79197          174         19.55 +/- 0.29
w2               77203        78103          886         20.05 +/- 0.14

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).