GCN Circular 7518

P. J. Brown and L. Vetere (PSU) report on behalf
of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field
of GRB 080325 (trigger=307604) starting 163 s after
the BAT trigger (Vetere et al., GCN Circ. 7512
Not found
 
 
).
We do not detect an optical/uv afterglow at the
enhanced XRT position (Osborne et al., GCN Circ. 7513
Not found
 
 
),
or NIR candidate (Updike et al., GCN Circ. 7515
Not found
 
 
) in
the initial finding chart observations or subsequent
summed images down to the following 3 sigma upper limits:

Filter    T_start (s) T_stop  Exposure      MagLimit
 white        163        262       98     >20.6
 white        163       5905      392     >21.5
   v          269        513      240     >19.3
   v          269       6297      419     >19.6
   b         5501       5700      197     >20.6
   u         4131      22211      353     >20.9
   uvw1      3925      21975     2371     >21.8
   uvm2      3720      10211      891     >21.1
   uvw2      5912       6111      197     >20.1

The above magnitudes are not corrected for the Galactic
extinction corresponding to a reddening of
E(B-V) = 0 .064 mag (Schlegel et al.,1998, ApJS, 500, 525).
The photometry is on the UVOT flight systemdescribed in
Poole et al. (2008, MNRAS, 383,627).