GCN CIRCULAR 1439
XRF 020427, detection of an underlying system with the VLT
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A. J. Castro-Tirado and J. Gorosabel, (Instituto de Astrofísica de Andalucía,
IAA-CSIC, Granada)
C. Sánchez-Fernández (ESA-VILSPA, Madrid)
N. Lund and S. Brandt (DSRI, Copenhagen)
J. M. Castro Cerón (ROA, San Fernando)
communicate:
"We have observed the field of the XRF 020427 (GCN 1383, 1384, 1386, 1390,
1394) on 11.388-11.397 June 2002 with the 8.2-m VLT telescope at Paranal
ESO's observatory (equipped with FORS2). Imagery was obtained in the B-
and R-bands (300-s exposure time each) under rather poor seeing conditions
(1".2). The position of the likely X-ray afterglow detected by BSAX and
followed-up by Chandra (GCN 1387, 1392) is coincident with the north part
of a extended (about 4" x 2"), blue object with R = 23.3 +/- 0.2 and
B = 23.8 +/- 0.4 which is consistent with the galaxy system reported
independently by Fruchter et al. (GCN Circ. 1440). An identification chart
is posted at www.iaa.es/~ajct/XRFs/xrf020427"