[vsnet-grb-info 3516] GRB 060719: Swift/UVOT Upper Limits

[GCN Circulars]

TITLE:   GCN GRB OBSERVATION REPORT
NUMBER:  5351
SUBJECT: GRB 060719: Swift/UVOT Upper Limits
DATE:    06/07/19 20:35:05 GMT
FROM:    Adam Morgan at PSU/Swift-UVOT  <qmorgan at gmail.com>

------=_Part_161248_15992668.1153341322351
Content-Type: text/plain; charset=ISO-8859-1; format=flowed
Content-Transfer-Encoding: 7bit
Content-Disposition: inline

A. Morgan, P. Brown (PSU), M. Stamatikos (GSFC/ORAU) on
behalf of the Swift/UVOT team:

The Swift UVOT began taking data on the field of GRB
060719 67 s after the BAT trigger (Stamatikos et al.,
GCN 5339).  No new source, relative to the DSS, is seen
inside the refined XRT error circle (Conciatore et al.,
GCN 5348).  The 3-sigma upper limits for the first finding
charts and the coadded images are listed below.

Finding charts:

Filter  Midpoint (s)  Exposure (s)    3-sigma UL
White   137           100             19.84
V       392           400             19.21

Coadded images:

Filter  T_range(s)    EXPOSURE (s)    3-sigma UL
White   87-17818      2240            21.68
V       67-22697      2117            20.27
B       669-16906     1298            21.15
U       646-6461      432             19.88
UVW1    622-24096     912             20.52
UVM2    598-23601     1279            21.15
UVW2    699-18307     1558            21.18

T_range is calculated from the time of the burst. These
upper limits have not been corrected for the estimated
Galactic reddening of E_{B-V} = 0.066 mag (Schlegel et
al. 1998).

------=_Part_161248_15992668.1153341322351
Content-Type: text/html; charset=ISO-8859-1
Content-Transfer-Encoding: 7bit
Content-Disposition: inline

A. Morgan, P. Brown (PSU), M. Stamatikos (GSFC/ORAU) on <br>
behalf of the Swift/UVOT team:<br>
<br>
The Swift UVOT began taking data on the field of GRB <br>
060719 67 s after the BAT trigger (Stamatikos et al., <br>
GCN 5339).&nbsp; No new source, relative to the DSS, is seen <br>
inside the refined XRT error circle (Conciatore et al., <br>
GCN 5348).&nbsp; The 3-sigma upper limits for the first finding <br>
charts and the coadded images are listed below. <br>
<br>
Finding charts:<br>
<br>
Filter&nbsp; Midpoint (s)&nbsp; Exposure (s)&nbsp;&nbsp;&nbsp; 3-sigma UL<br>
White&nbsp;&nbsp;
137&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
100&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
19.84&nbsp; &nbsp;<br>
V&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
392&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
400&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
19.21 &nbsp;<br>
<br>
Coadded images:<br>
<br>
Filter&nbsp; T_range(s)&nbsp;&nbsp;&nbsp; EXPOSURE (s)&nbsp;&nbsp;&nbsp; 3-sigma UL<br>
White&nbsp;&nbsp; 87-17818&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
2240&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
21.68<br>
V&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
67-22697&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
2117&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
20.27<br>
B&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp; 669-16906&nbsp;&nbsp;&nbsp;&nbsp;
1298&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
21.15<br>
U&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
646-6461&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
432&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
19.88<br>
UVW1&nbsp;&nbsp;&nbsp; 622-24096&nbsp;&nbsp;&nbsp;&nbsp;
912&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
20.52<br>
UVM2&nbsp;&nbsp;&nbsp; 598-23601&nbsp;&nbsp;&nbsp;&nbsp;
1279&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
21.15<br>
UVW2&nbsp;&nbsp;&nbsp; 699-18307&nbsp;&nbsp;&nbsp;&nbsp;
1558&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;&nbsp;
21.18<br>
<br>
T_range is calculated from the time of the burst. These <br>
upper limits have not been corrected for the estimated <br>
Galactic reddening of E_{B-V} = 0.066 mag (Schlegel et<br>
al. 1998).<br>
<br>

------=_Part_161248_15992668.1153341322351--