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 that a spectrogram (range 320-1000 nm) of 2006H (IAUC 8660), obtained on Jan. 20.3 UT under poor seeing conditions with the Supernova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope, shows it to be a type-Ia supernova. Its spectrum is similar to the peculiar, subluminous SN 1991bg (Filippenko et al. 1992, A.J. 104, 1543) at two days past maximum light. An approximate redshift of z about 0.01 is obtained from a fit to the supernova features.