GCN Circular 5822
A. C. Updike, B. C. Donehew, and D. H. Hartmann (Clemson University) report on behalf of the Clemson GRB Follow-Up Team: Using the Kitt Peak 2.1m telescope and FLAMINGOS NIR imaging and spectroscopy instrument, we imaged the field of GRB 060605. Under fair conditions, we integrated for two hours in the J band. At the location of the optical afterglow (GCN 5222), we do not detect the host galaxy to a limiting magnitude of 17.4. The Clemson University GRB Response Site can be found at: http://people.clemson.edu/~kgarime/burst/index.php This message may be cited.