[Message Prev][Message Next][Thread Prev][Thread Next][Message Index][Thread Index]
[vsnet-grb-info 361] GRB 020819: Optical observations
TITLE: GCN GRB OBSERVATION REPORT
NUMBER: 1511
SUBJECT: GRB 020819: Optical observations
DATE: 02/08/20 16:01:13 GMT
FROM: Paul Price at RSAA, ANU <pap@mso.anu.edu.au>
P.A. Price (RSAA, ANU), D.W. Fox (Caltech), A. Piccioni, C. Bartolini,
I. Bruni, R. Gualandi., A. Guarnieri (Bologna University and Bologna
Astronomical Observatory), G. Pizzichini (IASF-CNR, Sezione di Bologna)
and R. McNaught (RSAA, ANU) report:
We observed the SXC error-circle of GRB 020819 (GCN #1508) with the
Palomar 60-inch telescope at Aug 20.34 UT with 4x600 sec exposures in R.
Comparison of this combined image with those from the SSO 40-inch
telescope (GCN #1506) and the Loiano 1.5-metre telescope (GCN #1509),
both visually and through image subtraction do not reveal any afterglow
candidates. We estimate the limiting magnitudes to be as follows:
SSO 40-inch R ~ 20.5 mag (GCN #1506)
Loiano 1.5-metre R ~ 21.7 mag (GCN #1509)
Palomar 60-inch R ~ 21.5 mag
Comparison of the best NIR afterglow candidate (GCN #1510) with other
sources in the field suggests that this candidate is likely constant in
flux.
This message may be cited.
Return to Daisaku Nogami
vsnet-adm@kusastro.kyoto-u.ac.jp