[vsnet-grb-info 8145] GRB 090715B: Swift/UVOT followup observations

GCN Circulars gcncirc at capella.gsfc.nasa.gov
Thu Jul 16 21:32:15 JST 2009


TITLE:   GCN CIRCULAR
NUMBER:  9678
SUBJECT: GRB 090715B: Swift/UVOT followup observations
DATE:    09/07/16 12:32:09 GMT
FROM:    Alice Breeveld at MSSL-UCL  <aab at mssl.ucl.ac.uk>

A. Breeveld (MSSL/UCL) and L. Vetere (PSU)
report on behalf of the Swift/UVOT team:

The Swift/UVOT began settled observations of the field of GRB 090715B
53 s after the BAT trigger (Vetere et al., GCN Circ. 9668).
The optical afterglow reported in Vetere et al., GCN 9668 and  
confirmed by Smith et al., GCN 9670, Malesani et al., GCN 9671,  
Wiersema et al., GCN 9673 and Antonelli et al., GCN 9675 is detected  
by the UVOT only in the initial white exposure. The detected magnitude  
and preliminary 3-sigma upper limits obtained using a 3" aperture and  
the UVOT photometric system
(Poole et al. 2008, MNRAS, 383, 627) for the first finding chart (FC)
exposure and subsequent summed exposures are:

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

white_FC         53            203          147         20.37 +/- 0.15
white            4052         4252          196         >21.3
v                    5989       22687          795         >21.0
b                    3848         4047          197         >20.3
u                      266       16495          428         >21.2
w1              12053       16278          894         >21.2
m2                6195       10367          826         >21.0
w2                4258       22065          995         >21.4

The values quoted above are not corrected for the Galactic extinction
due to the reddening of E(B-V) = 0.01 in the direction of the burst
(Schlegel et al. 1998).


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