TITLE: GCN CIRCULAR NUMBER: 18831 SUBJECT: GRB 160104A: Spectroscopic observations from 10.4m GTC DATE: 16/01/05 12:09:05 GMT FROM: Antonio de Ugarte Postigo at IAA-CSIC A. de Ugarte Postigo (IAA-CSIC, DARK/NBI), C.C. Thoene (IAA-CSIC), J.P.U. Fynbo (DARK/NBI), N.R. Tanvir (U. Leicester), R. Sanchez-Ramirez (IAA-CSIC) and S. Geier (GRANTECAN), report on behalf of a larger collaboration: We observed the afterglow of GRB 160104A (Melandri et al. GCN18815, Guidorzi et al. GCN18816) with OSIRIS on the 10.4 m GTC telescope, located at the Roque de los Muchachos Observatory (La Palma, Spain). Observations started at 20:25 UT (9.0 hr after the GRB onset) and consisted of a 40 s acquisition image in i-band as well as 3x900s spectra using the R1000R grism which covers the range between 5100 and 10000 AA with a resolution of R~800. The acquisition image was obtained under good conditions with a seeing of 0.8". The afterglow is clearly detected although it shows a strong decay in brightness with respect to previous detections (Guidorzi et al. GCN18816, Saito et al. GCN 18817, Yurkov et al. GCN 18820, Xin et al. 18823). As compared to USNO-B1.0 stars we measure a magnitude of i(Vega)=22.6, roughly equivalent to i(AB)=23.0. The combined spectrum shows a clear continuum over the complete range with only one prominent absorption feature centred at 5889 AA, with an equivalent width of ~30 AA. There are also tentative absorptions features at ~5300 and ~5340 AA. There is no drop bluewards of the 5889 AA feature which could otherwise be suggestive of a weak Ly-alpha at z=3.84. At a redshift of 2.80, the features could be consistent with CIV and the two SiIV, respectively. We are not able to establish a convincing solution for the redshift based on this evidence.