NOTE: uvot_fluxes_wget.pl vrs. 2018-01-16 fem at 180205d23h57m28s587441usUT
NOTE: Source region spec. is: 126.8196 +11.5418 3"
NOTE: Used archived uvot source position of 126.81960  11.54180  3.00
NOTE: position reference is GCN_Notice
NOTE: A UVOT position was reported in GCN_Notice_Mon_05_Feb_18_04:35:32_UT
NOTE: Possible detection in uu at T+490.3
NOTE: Possible detection in wh at T+181.5
NOTE: Possible detection in bb at T+515.0
NOTE: Possible detection in w1 at T+465.9
NOTE: Possible detection in vv at T+158.3
NOTE: Possible detection in w2 at T+391.4
NOTE: Possible detection in m2 at T+440.9
WARNING: t_start for light curve (158) and t_start from the exposure report (138) do not agree.
  Replace ??? in draft Circular with correct value.

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

GRB 180205A: Swift/UVOT Upper Limits

S.W.K. Emery (UCL-MSSL) and ***BA*** (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 180205A
***???*** s after the BAT trigger (***Author*** et al., GCN Circ. ????).
No optical afterglow consistent with the XRT position
*** POSITION REFERENCE is GCN_Circ-22381 ***
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           182          331          147         >15.7
white              182         6473          380         >16.6
v                  158        11825         1134         >18.3
b                  515         6268          236         >17.8
u                  490         6063          236         >17.1
w1                 466         5858          236         >17.0
m2                 441        12726         1117         >18.4
w2                 391         6676          429         >18.7

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.03 in the direction of the burst
(Schlegel et al. 1998).


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

GRB 180205A: Swift/UVOT Detection

S.W.K. Emery (UCL-MSSL) and ***BA*** (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 180205A
***???*** s after the BAT trigger (***Author*** et al., GCN Circ. ????).
A source consistent with the XRT position
*** POSITION REFERENCE is GCN_Circ-22381 ***
is detected in the initial UVOT exposures.

The preliminary UVOT position is:
    RA  (J2000) =  08:27:16.74 = 126.81975 (deg.)
    Dec (J2000) = +11:32:30.9  =  11.54191 (deg.)
with an estimated uncertainty of 0.42 arc sec. (radius, 90% confidence).

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              182          331          147         15.75 +/- 0.02
v                  158          172           13         16.18 +/- 0.16
b                  515          535           20         16.71 +/- 0.09
u                  490          510           19         15.70 +/- 0.08
w1                 466          486           19         15.78 +/- 0.13
m2                 441          461           20         15.90 +/- 0.18
w2                 391          585           39         17.08 +/- 0.18

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.03 in the direction of the burst
(Schlegel et al. 1998).