NOTE: uvot_fluxes_wget.pl vrs. 2018-11-07 fem at 200614d03h59m35s163718usUT
NOTE: Source region spec. is: 153.04083 45.75414 4"
NOTE: Used archived XRT position of 153.04083  45.75414  4.00
NOTE: position reference is GRB_Auto_Processing
NOTE: Possible detection in uu at T+43621.0
NOTE: Possible detection in wh at T+50196.6

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

GRB 200613A: 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 200613A
43621 s after the LAT trigger (***Author*** et al., GCN Circ. ????).
No optical afterglow consistent with the XRT position
*** POSITION REFERENCE is GRB_Auto_Processing ***
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            50197        56308         1173         >19.5
v                50992        51208          213         >18.6
u                43621        62180         2355         >18.8

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 200613A: 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 200613A
43621 s after the LAT trigger (***Author*** et al., GCN Circ. ????).
A source consistent with the XRT position
*** POSITION REFERENCE is GRB_Auto_Processing ***
is detected in the initial UVOT exposures.

The preliminary UVOT position is:
    RA  (J2000) =  10:12:10.03 = 153.04178 (deg.)
    Dec (J2000) = +45:45:14.1  =  45.75391 (deg.)
with an estimated uncertainty of 0.46 arc sec. (radius, 90% confidence).

Preliminary detections and 3-sigma upper limits 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            50197        50985          775         19.65 +/- 0.07
v                50992        51208          213        >18.6
u                49402        50190          775         19.02 +/- 0.12

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).