[vsnet-grb-info 9122] GRB 100414A: Swift/UVOT Observations
GCN Circulars
gcncirc at capella.gsfc.nasa.gov
Sun Apr 18 00:56:50 JST 2010
TITLE: GCN CIRCULAR
NUMBER: 10609
SUBJECT: GRB 100414A: Swift/UVOT Observations
DATE: 10/04/17 15:56:44 GMT
FROM: Wayne Landsman at GSFC/SSAI <wayne.b.landsman at nasa.gov>
W. Landsman (GSFC) and J. Cannizzo (GSFC) report on behalf of the
Swift/UVOT team:
The Swift/UVOT began observations of the field of GRB 100414A 40.4 hours
after the Fermi LAT and GBM-detected trigger (Takahashi et al. GCN Circ.
10594, Foley et al., GCN Circ. 10595). We detect the source reported
by Cucchiara & Fox (GCN Circ. 10606, 10608) and Filgas et al. (GCN Circ.
10607) Combining our white observations into exposures beginning at
40.4 and 53.2 hours, we find evidence for source fading.
Filter T_start (hr) Exp(s) Mag Err
White 40.38 765 20.54 +/- 0.10
White 53.20 3531 20.86 +/- 0.06
These observations are not corrected for the expected Galactic
foreground extinction corresponding to a reddening of E_(B-V)=0.03 mag
in the direction of the burst (Schlegel et al. 1998). The photometry
is on the UVOT photometric system described in Poole et al.(2008, MNRAS,
383,627).
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