TITLE: GCN CIRCULAR NUMBER: 12770 SUBJECT: GRB 111228A: X-shooter spectroscopy DATE: 11/12/29 19:19:59 GMT FROM: Steve Schulse at U. of Iceland S. Schulze (U Iceland), S. Covino (INAF-OABr), H. Flores (GEPI/Obs. de Paris), J. P. U. Fynbo (DARK/NBI), B. Milvang-Jensen (DARK/NBI), J. Sollerman (U Stockholm), D. Xu (WIS) report on behalf of the X-shooter GRB collaboration: We observed the afterglow of GRB 111228A (Ukwatta et al. GCN 12737) with the ESO VLT equipped with the X-shooter spectrograph on 29 December 2011, beginning 07:40 UT (15.93 hr after the GRB). The afterglow had an R-band brightness of 20.08 mag in a series of five acquisition images with an exposure time of 30 s each (mid-exposure time = 15.98 hours). The magnitude is not corrected for Galactic extinction. We acquired four spectra with an exposure time of 600 seconds each, beginning at 07:47 UT. We detect several absorption lines wave_obs wave_rest Ion redshift (AA, vac) (AA, vac) 3880.28 2260.78 FeII 0.71634 4023.15 2344.21 FeII 0.71620 4075.26 2374.46 FeII 0.71629 4089.47 2382.77 FeII 0.71627 4422.70 2576.88 MnII 0.71630 4439.44 2586.65 FeII 0.71629 4453.10 2594.50 MnII 0.71636 4462.57 2600.17 FeII 0.71626 4799.05 2796.35 MgII 0.71618 4811.32 2803.53 MgII 0.71616 4896.33 2852.96 MgI 0.71623 6753.24 3934.78 CaK 0.71630 6813.09 3969.59 CaH 0.71632 at a common redshift of z = 0.71627 +/- 0.00002. In addition we detect [OIII]5007 at z_em = 0.71635, similar to the absorption line redshift. Our measurements confirm the results by of Cucchiara et al (GCN 12761) and Palazzi et al (GCN 12763) and are similar to Dittmann et al (GCN 12759) and Xu et al (GCN 12764). The seeing conditions over the entire campaign were around 0.8 arcsec. We acknowledge the support of the VLT staff, in particular Claudio Melo and Christophe Martayan.