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![]() TITLE: GCN CIRCULAR NUMBER: 7444 SUBJECT: VLT/UVES redshift of GRB 080319B DATE: 08/03/19 13:34:33 GMT FROM: Paul Vreeswijk at Dark Cosmology Centre,U.of Copenhagen <pmv@dark-cosmology.dk> P. M. Vreeswijk (DARK), A. Smette (ESO), D. Malesani, J. P. U. Fynbo, Bo Milvang-Jensen (DARK), P. Jakobsson (U. Hertfordshire), A. O. Jaunsen (U. Oslo), and C. Ledoux (ESO) report on behalf of a larger collaboration: We observed the optical afterglow of GRB 080319B (Racusin et al., GCN 7427) with the Ultraviolet and Visual Echelle Spectrograph (UVES) mounted at ESO's VLT Kueyen. Observations were performed in rapid-response mode starting on 2008 March 19 at 07:18 UT. The highest redshift system that we identify based on the MgII doublet and various other features has z=0.937, the presumed redshift of GRB 080319B. Another system is identified at z=0.530. We acknowledge excellent support from the observing staff at Paranal,
in particular Swetlana Hubrig and Elena Mason. Cited by 6 messages Spectral Observations
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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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