SIMBAD references

The "Nearby Supernova Factory" collaboration (N. Blanc, Y. Copin, E. Gangler, 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; G. Aldering, S. Bailey, S. Bongard, D. Kocevski, S. Loken, P. Nugent, S. Perlmutter, R. Scalzo, R. C. Thomas, L. Wang, and B. A. Weaver, Lawrence Berkeley National Laboratory; 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 that a spectrum (range 320-1000 nm) of SN 2006au (cf. CBET 426), obtained under bad seeing conditions on Mar. 13.6 UT with the University of Hawaii 2.2-m telescope (+ Supernova Integral Field Spectrograph), shows it to be a type-II supernova at an approximate redshift of z = 0.01, consistent with that of the host (UGC 11057, z = 0.009580; Theureau et al. 1998, A.Ap. Suppl. 130, 333, via NED). The spectrum shows a well-developed H-alpha P-Cyg profile.