SIMBAD references

C. J. Stockdale and M. Kelley, Marquette University; S. D. Van Dyk, Spitzer Science Center, California Institute of Technology; R. A. Sramek, National Radio Astronomy Observatory; K. W. Weiler, Naval Research Laboratory; and N. Panagia, European Space Agency, report the lack of detection of radio emission near the position of the type-II SN 2005cs (IAUC 8553, 8555) with the Very Large Array. Upper limits (3 sigma) to any radio flux density were established on the following dates: July 2.01 UT, < 0.585 mJy at 22.460 GHz (wavelength lambda = 1.3 cm); 3.00, < 0.900 mJy at 14.940 GHz (lambda = 2.0 cm) and < 0.189 mJy at 8.460 GHz (lambda = 3.5 cm); 8.968, < 0.291 mJy at 8.460 GHz and < 0.918 mJy at 22.460 GHz; 22.038 < 0.161 mJy at 8.460 GHz and < 0.464 mJy at 22.460 GHz; Aug. 9.00, < 0.129 mJy at 8.460 GHz; 14.837, < 0.187 mJy at 8.460 GHz and < 0.372 mJy at 4.860 GHz (lambda = 6.2 cm). The search for radio emission was conducted within about 10" of the published optical position of SN 2005cs (R.A. = 13h29m52s.78, Decl. = +47o10'35".7, equinox 2000.0; cf. IAUC 8553), and no radio emission was detected near the supernova position exceeding three times the map rms at any of the times or in any of the frequency bands listed.