[AAVSO-HEN] GRB 090205: VLT optical decay
grb at aavso.org
grb at aavso.org
Sat Feb 7 04:35:35 EST 2009
The following is a GCN Circular circulated via the AAVSO network.
For an archive and more information on circulars visit:
http://lheawww.gsfc.nasa.gov/docs/gamcosray/legr/bacodine/gcn3_archive.html
TITLE: GCN CIRCULAR
NUMBER: 8895
SUBJECT: GRB 090205: VLT optical decay
DATE: 09/02/07 09:35:05 GMT
FROM: Paolo D'Avanzo at INAF-OAB <paolo.davanzo at brera.inaf.it>
P. D'Avanzo, D. Fugazza (INAF-OAB), V. D'Elia (INAF-OAR), R. Salvaterra,
C. C. Thoene (INAF-OAB), S. Piranomonte (INAF-OAR), S. Covino, S.
Campana (INAF-OAB), G. Chincarini (Univ. Bicocca) report, on behalf of
the MISTICI collaboration:
We continued monitoring GRB 090205 (Perri et al., GCN 8884) with the
ESO-VLT in imaging mode. Observations were carried out in R-band with
the FORS1 camera about 1.35 days after the burst.
Preliminary analysis of a first set of images (total exposure: 12 min)
reveals that the optical afterglow (D'Avanzo et al. GCN 8887; Kruehler &
Greiner GCN 8888) is still detected and that it faded by about 3 mags
with respect to our previous epoch of VLT observations (D'Avanzo et al.
GCN 8887). Assuming a power-law decy, the inferred decay index between
this two epochs is alpha ~ 1.8, steeper than what measured in the X-rays
at earlier epochs (Perri & Stratta, GCN 8891). Further optical
observations are ongoing.
We acknowledge the VLT staff for their support, in particular G. James
and L. Schmidtobreick.
More information about the Aavso-hen
mailing list