Table 3: UVOT multicolour data.
Filter T(mid) T(expo) Magnitudea Flux densityb
  (s) (s) (mag)  
V 183.40 153.31 $16.96 \pm 0.08$ $0.522 \pm 0.038$
V 632.99 725.22 $16.79 \pm 0.04$ $0.610 \pm 0.022$
B 11 477.47 139.43 $18.60 \pm 0.12$ $0.220 \pm 0.024$
B 17 915.40 884.89 $19.05 \pm 0.06$ $0.145 \pm 0.008$
B 23 674.52 884.87 $19.51 \pm 0.08$ $0.095 \pm 0.007$
B 29 314.24 884.85 $19.53 \pm 0.09$ $0.093 \pm 0.008$
V 35 202.82 1573.78 $19.30 \pm 0.09$ $0.060 \pm 0.005$
V 41 022.66 1575.25 $19.44 \pm 0.10$ $0.053 \pm 0.005$
V 46 782.58 1575.15 $19.52 \pm 0.10$ $0.049 \pm 0.005$
V 58 332.60 4725.17 $19.62 \pm 0.07$ $0.045 \pm 0.003$
V 75 672.93 4752.29 $19.86 \pm 0.08$ $0.036 \pm 0.003$
V 99 028.58 7947.60 $20.15 \pm 0.08$ $0.028 \pm 0.002$
a Vega magnitudes. b In units of 10-16 erg cm-2 s-1 $\AA^{-1}$.
Note. Errors are 1-$\sigma$ values. rms errors in the photometric zero points have not been included. UVOT magnitudes were not corrected for Galactic extinction. Mid times are measured since the BAT trigger.

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