GCN Circular 2314
Subject
XRF 030723, optical observations
Date
2003-07-23T23:55:59Z (21 years ago)
Edited On
2024-11-18T09:44:00Z (a month ago)
From
Alberto Castro-Tirado at LAEFF-INTA <ajct@laeff.esa.es>
Edited By
Judith Racusin at NASA/GSFC <judith.racusin@nasa.gov> on behalf of Leo P. Singer at NASA/GSFC <leo.p.singer@nasa.gov>
XRF 030723, optical observations
-------------------------
A. de Ugarte (IAA-CSIC, Granada), P. Tristram (Univ. of
Auckland), T. Sekiguchi (Univ. of Nagoya), M. Jelinek
(ASU-CAS, Obs. Ondrejov), J. Gorosabel (IAA-CSIC and
STScI, Baltimore), S. Guziy (IAA-CSIC), J. M. Castro
Cerón (STScI), P. Kilmartin (Mt. John Obs.), Ph. Yock
(Univ. of Auckland) and A. J. Castro-Tirado (IAA-CSIC)
communicate:
"Following the detection of the X-ray flash 030723 by
HETE-2, we have imaged the entire error box with the
0.6-m telescope (+MOA camera) at Mt. John Observatory
in wide R- and B-band filters (3 x 300-s each) starting
on July 23.59 UT (i.e. 7.6 hr after the event).
Comparison of a single R-band frame with the DSS-2 (R-
-band) reveals no optical transient down to the DSS-2
limiting magnitude."