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![]() TITLE: GCN CIRCULAR NUMBER: 9403 SUBJECT: GRB 090519: NOT afterglow candidate DATE: 09/05/19 22:32:39 GMT FROM: Daniele Malesani at Dark Cosmology Centre, Niels Bohr Inst <malesani@astro.ku.dk> C. C. Thoene (INAF/Brera), D. Malesani (DARK/NBI), A. J. Levan (Univ. Warwick), P. Jakobsson (Univ. Iceland), J. Hjorth (DARK/NBI), and N. R. Tanvir (Univ. Leicerster), report on behalf of a larger collaboration We observed the field of GRB 090519 (Perri et al.
, GCN 9400) with the
NOT equipped with ALFOSC.
At the edge of the XRT error circle, we detect a fading source at
coordinates (J2000):
RA = 09:29:07.0
Dec = +00:10:49.1
with an error of ~0.5". The source faded by ~0.3 +- 0.10 mag between
19.8 and 44.4 min after the GRB, suggesting that this is indeed the
afterglow of GRB 090519. A (fainter) object is seen at the position of
the candidate in the SDSS, which may be a bright host galaxy. On May
19.897 UT, the source had R ~ 21.6. Cited by 4 messages
This site was created by Robert Quimby
Database maintained by Robert Quimby, Erin McMahon, and Jeremy Murphy Information displayed on this site is compiled from GCN Circulars and other sources as indicated. |
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