GCN Circular 6419
Subject
GRB070518: UVOT refined analysis
Date
2007-05-19T03:18:58Z (18 years ago)
From
Antonino Cucchiara at PSU <cucchiara@astro.psu.edu>
Cucchiara A. (PSU), Marshall F. E. (NASA/GSFC) and Guidorzi C.
(Univ. Bicocca&INAF-OAB) reports on behalf of the Swift/UVOT team:
The Swift/UVOT observed the field of GRB070518 starting
82 sec after the trigger (Guidorzi et al., GCN Circ. 6415).
The afterglow was clearly detected in all the 7 filters.
This suggest a redshift lower than 0.7.
The estimated magnitude for the V and White filters are:
Filter T_start(sec) Exposure(sec) Mag
White 82 93 18.16 +/- 0.06
White 873 94 19.14 +/- 0.09
White 5517 191 20.08 +/- 0.14
White 6951 191 21.33 +/- 0.20
V 187 391 19.31 +/- 0.13
V 978 391 20.08 +/- 0.24
V 5927 363 21.05 +/- 0.48
Assuming a single power-low, the decay index is ~1.17 in V band.
The extrapolated V mag at T+10h is 22.59.
The values quoted above are not corrected for the expected Galactic
extinction of E_{B-V} = 0.017 mag (Schlegel et al. 1998).