NOTE: uvot_fluxes_wget.pl vrs. 2018-11-07 fem at 190324d17h36m44s270326usUT
NOTE: Source region spec. is: 40.13296 61.22894 4"
NOTE: Used archived XRT position of  40.13296  61.22894  4.00
NOTE: position reference is GRB_Auto_Processing
NOTE: Possible detection in uu at T+302.0
NOTE: Possible detection in wh at T+89.5
NOTE: Possible detection in bb at T+557.6
NOTE: Possible detection in w1 at T+681.9
NOTE: Possible detection in vv at T+632.1
NOTE: Possible detection in w2 at T+607.6
NOTE: Possible detection in m2 at T+657.1

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

GRB 190323: Swift/UVOT Upper Limits

J. D. Gropp (PSU) and ***BA*** (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 190323
90 s after the BAT 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 first
finding chart (FC) exposure and subsequent exposures are:

Filter         T_start(s)   T_stop(s)      Exp(s)         Mag

white_FC            90          239          147         >15.0
u_FC               302          552          246         >11.6
white               90         6274          626         >14.8
v                  632         6489          179         >11.1
b                  558         6069          352         >12.8
u                  302         5863          579         >11.7
w1                 682         5658          333         >12.0
m2                 657         2126          172         >13.2
w2                 608         6480          372         >12.9

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 1.54 in the direction of the burst
(Schlegel et al. 1998).


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

GRB 190323: Swift/UVOT Detection

J. D. Gropp (PSU) and ***BA*** (***BA INSTITUTION***)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 190323
90 s after the BAT 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.

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               90          239          147         15.00 +/- 0.02
v                  632          652           20         11.14 +/- 0.06
b                  558          577           20         12.42 +/- 0.06
u                  302          552          246         11.62 +/- 0.02
w1                 682          702           20         12.00 +/- 0.04
m2                 657          677           20         13.18 +/- 0.06
w2                 608          627           20         12.75 +/- 0.04

The magnitudes in the table are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 1.54 in the direction of the burst
(Schlegel et al. 1998).