GCN Circular 6398
Subject
GRB 070508: OA fading and tentative redshift
Event
Date
2007-05-09T15:11:02Z (18 years ago)
From
Pall Jakobsson at U Hertfordshire <P.Jakobsson@herts.ac.uk>
Pall Jakobsson (U. Hertfordshire), Johan P. U. Fynbo (DARK, NBI),
Michael I. Andersen (Potsdam), Andreas O. Jaunsen (U. Oslo),
Christina C. Thoene, Darach Watson, Jens Hjorth, Bo Milvang-Jensen
(DARK, NBI), Nial R. Tanvir (U. Leicester) and P. Moller (ESO)
report on behalf of a larger collaboration:
Using FORS1 on the Very Large Telescope, we have obtained 3*30 min
spectra (grism 300V) of GRB 070508 (Grupe et al., GCN 6383). The
UVOT optical afterglow candidate (Marshall & Grupe, GCN 6392) has
clearly faded in our acquisition image. Using photometric zeropoints
from the ESO webpages we estimate the afterglow magnitude to be
R ~ 22.0 on May 8.337 (3.79 hours post-burst).
The combined spectrum does not display any obvious absorption
features. However, a firm upper limit of z < 2.3 can be placed on
the redshift of GRB 070508 from the lack of Ly-alpha forest lines in
the spectrum of the afterglow. This is consistent with the UVOT
observations (Marshall & Grupe, GCN 6392).
We do detect a tentative emission line at 6781 A. If it corresponds
to H-alpha at z = 0.033, we would expect to detect H-beta and the
[O III] doublet in our spectrum. However, no features are visible
at their predicted locations. The most probable association is with
[O II] 3728, corresponding to a redshift of z = 0.82. We caution
that the magnitude reported above is then most likely affected by
host galaxy emission.
We thank the Paranal staff for excellent support.