SIMBAD references

The "Nearby Supernova Factory" collaboration (G. Aldering, S. Bailey, S. Bongard, D. Kocevski, B. C. Lee, S. Loken, P. Nugent, S. Perlmutter, R. Scalzo, R. C. Thomas, L. Wang, and B. A. Weaver, Lawrence Berkeley National Laboratory, Berkeley; N. Blanc, Y. Copin, E. Gangler, L. Sauge, and G. Smadja, Institut de Physique Nucleaire de Lyon; P. Antilogus, S. Gilles, R. Pain, and R. Pereira, Laboratoire de Physique Nucleaire et de Haute Energies de Paris; E. Pecontal and G. Rigaudier, Centre de Recherche Astronomique de Lyon; R. Kessler, Kavli Institute for Cosmological Physics, Chicago; and C. Baltay, D. Rabinowitz, and A. Bauer, Yale University) reports the discovery of three supernovae in NEAT images obtained using the Palomar Oschin 1.2-m telescope (+ QUEST II camera). Discovery-image dates and approximate magnitudes (calibrated to R) are listed in the table below. Spectroscopy (range 320-1000 nm) of these objects were obtained on Jan. 18.5-18.6 UT with the University of Hawaii 2.2-m telescope (+ Supernova Integral Field Spectrograph); redshifts were derived from the peak of the observed H_alpha emission: 2006K, z = 0.03; 2006L, 0.04; 2006M in PGC 47137, 0.015. The host galaxy of 2006L, 2MASX J13070825+2838003, has z = 0.03940 (measured by Wegner et al. 2003, A.J. 125, 2373; via NED); PGC 47137 has z = 0.01544 (measured by Rines et al. 2003, A.J. 126, 2152; via NED). SN 2006 UT R.A. (2000.0) Decl. Mag. Type 2006K Jan. 17.5 11 29 46.26 -17 25 17.8 18.6 II 2006L Jan. 17.6 13 07 11.76 +28 38 46.2 19.9 IIn 2006M Jan. 17.6 13 27 19.76 +31 47 14.5 18.5 II