[AAVSO-HEN] GRB 080810: optical observations
grb at aavso.org
grb at aavso.org
Wed Dec 24 09:22:18 EST 2008
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: 8722
SUBJECT: GRB 080810: optical observations
DATE: 08/12/24 14:21:54 GMT
FROM: Alexei Pozanenko at IKI, Moscow <apozanen at iki.rssi.ru>
A. Volnova (SAI MSU), I. Korobtsev (ISTP), A. Pozanenko (IKI), E. Klunko
(ISTP), N. Bochkarev (SAI MSU), E. Karitskaja (Institute of Astronomy), on
behalf of larger GRB follow up collaboration report:
We observed the afterglow of GRB 080810 (Page et al. GCN 8080) with 1.5 m
telescope of Sayan observatory (Mondy) under good weather conditions.
Series of R and B images were obtained between Aug. 10 (UT)
16:50:03 -18:17:06. While we clearly detect afterglow in single R images,
the afterglow is not detected in a combined image obtained in B. A
photometry of the combined images is based on several SDSS nearby stars:
T0+ Filter Exp. mag. Upper_Limit seeing
mid., days (3 sigma)
0.1599 B 14x60 n/d 19.26 ~2.7"
0.1786 R 30x60 17.98 +/- 0.13 20.85 ~2.2"
0.2026 R 30x60 18.10 +/- 0.17 21.14 ~2.0"
The photometry in R-band is an agreement with power law decay index of
light curve (alpha = 1.12) between 400 s and 1 day after the burst reported
by Thoene et al (GCN 8106).
More information about the Aavso-hen
mailing list