SIMBAD references

The "Nearby Supernova Factory" collaboration (E. Pecontal and G. Rigaudier, Centre de Recherche Astronomique de Lyon; P. Antilogus, S. Gilles, R. Pain, and R. Pereira, Laboratoire de Physique Nucleaire et de Haute Energies de Paris; C. Buton, Y. Copin, E. Gangler, and G. Smadja, Institut de Physique Nucleaire de Lyon; G. Aldering, C. Aragon, S. Bailey, S. Bongard, M. J. Childress, S. Loken, P. Nugent, S. Perlmutter, K. Runge, R. Scalzo, R. C. Thomas, and B. A. Weaver, Lawrence Berkeley National Laboratory, Berkeley; R. Kessler, Kavli Institute for Cosmological Physics, Chicago; and C. Baltay, A. Bauer, D. Herrera, and D. Rabinowitz, Yale University) reports the discovery of an apparent supernova (mag approximately 16.0, calibrated to R) in images obtained on Oct. 19.3 UT the QUEST II camera on the Palomar Oschin 1.2-m Schmidt telescope as a part of the NEAT component (cf. CBET 263) of the Palomar-QUEST Consortium. The new object is located at R.A. = 0h35m27s.81, Decl. = +2d55'50".7 (equinox 2000.0). Nothing is visible at this location on an image taken on Sept. 20 (approximate limiting mag 20.0). The host galaxy, UGC 348, has z = 0.014 (Schneider et al. 1992, Ap.J. Suppl. 81, 5, via NED).