SIMBAD references

R. J. Beswick, D. Fenech, H. Thrall, M. K. Argo, T. W. B. Muxlow, and A. Pedlar, Jodrell Bank Observatory, report further detections of the radio emission from the evolving type-II supernova 2002hh in NGC 6946 (IAUC 8005, 8018) and limits on the radio emission from SN 2005V in NGC 2146. Very Large Array 'B'- configuration observations of 2002hh detected flux densities of 0.35 ± 0.1 mJy at 4.860 GHz on 2003 Nov. 14 and 1.6 ± 0.2 mJy at 1.425 GHz on 2005 Apr. 16 at R.A. = 20h34m44s.25, Decl. = +60o07'19".4 (equinox 2000.0; ± 0".2 in each coordinate), in close agreement with previously reported positions. MERLIN observations place 3-sigma upper limits for the type-Ib/c supernova 2005V (cf. IAUC 8474) on 2005 Apr. 4 of 0.14 mJy at 1.658 GHz, and on May 19 of 0.23 mJy at 1.408 GHz at the reported position. Further observations of both sources are underway.