NOTE: uvot_fluxes_wget.pl vrs. 2016-02-01 fem at 160914d02h48m07s861666usUT
NOTE: Used archived opt source position of 221.44183  39.06672  3.00
NOTE: position reference is GCN_Circ-19908
NOTE: Possible detection in wh at T+196954.6

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

GRB 160910A: Swift/UVOT Upper Limits

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

The Swift/UVOT began settled observations of the field of GRB 160910A
196955 s after the LAT trigger (***Author*** et al., GCN Circ. ????).
No optical afterglow consistent with the optical position
*** POSITION REFERENCE is GCN_Circ-19908 ***
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

white           196955       277128         2781         >20.6

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 160910A: Swift/UVOT Detection

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

The Swift/UVOT began settled observations of the field of GRB 160910A
196955 s after the LAT trigger (***Author*** et al., GCN Circ. ????).
A source consistent with the optical position
*** POSITION REFERENCE is GCN_Circ-19908 ***
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

white           225033       225588          546         20.80 +/- 0.18

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).