SIMBAD references

S. Ryder, Australian Astronomical Observatory; A. Soderberg, Harvard University; C. Stockdale, Marquette University; S. Van Dyk, Spitzer Science Center, California Institute of Technology; S. Immler, Goddard Space Flight Center; K. Weiler, Naval Research Laboratory; and N. Panagia, Space Telescope Science Institute and Observatory of Catania, report the detection of radio emission near the position of SN 2011ja with the Australia Telescope Compact Array radio telescope, confirming its core-collapse nature. A flux density of 0.44 ± 0.20 mJy was measured at 18.0 GHz on Dec 19.9 UT. The measured position of the radio emission of R.A. = 13:05:11.06, Decl. = -49:31:26.0 (equinox 2000.0) is in good agreement with the measured optical position (end figures 11s.12, 27".0). Radio observations of this nearby (4 Mpc, from NED) supernova at the Australia Telescope Compact Array are continuing.