TITLE: GCN CIRCULAR NUMBER: 6663 SUBJECT: GRB 060814 - Keck host detection and redshift DATE: 07/07/24 21:18:06 GMT FROM: Christina Thoene at Niels Bohr Institute,DARK Cosmo Ctr Christina C. Thoene (DARK/UC Berkeley), Daniel A. Perley and J. S. Bloom (UC Berkeley) report: On 2007 April 15 (UT) we imaged the field of GRB 060814 with Keck I 10m telescope + LRIS for 750s in I and 840s in V under poor seeing conditions. The host galaxy reported by Malesani et al. (GCN 5456) and others is well-detected at a position consistent with the locations of the IR (Levan et al., GCN 5455) and X-ray (GCN 5451; [1]) transients. A finding chart of the field can be found at: http://lyra.berkeley.edu/~dperley/060814/060814_lris_v.png We also took spectra of the host galaxy on July 18 with LRIS, using grism 600/4000 and dicroic 560, which covers the wavelength range between 5500 and 9700 AA in the red arm. From the detected [OII] 3729 AA and [OIII] 5008 AA emission lines, we infer a redshift of z=0.84 for the host galaxy. The second [OIII] line at 4959 is marginally detected whereas H beta lies in the atmospheric absorption lines and could not be detected. An image of the 2D spectrum indicating the detected emission lines can be found at: http://lyra.berkeley.edu/~cthoene/GRBs/GRB060814_2dspec.jpg footnote: [1] 14:45:21.29, +20:35:10.7, 90% unc. 0.9", from http://astro.berkeley.edu/~nat/swift/xrt_pos.html (v0.0)