SIMBAD references

The "Nearby Supernova Factory" collaboration (P. Antilogus, S. Gilles, R. Pain, and R. Pereira, Laboratoire de Physique Nucleaire et de Haute Energies de Paris; N. Blanc, Y. Copin, E. Gangler, and G. Smadja, Institut de Physique Nucleaire de Lyon; G. Aldering, C. Aragon, S. Bailey, S. Bongard, M. J. Childress, D. Kocevski, S. Loken, P. Nugent, S. Perlmutter, K. Runge, R. Scalzo, R. C. Thomas, L. Wang, and B. A. Weaver, Lawrence Berkeley National Laboratory, Berkeley; E. Pecontal and G. Rigaudier, Centre de Recherche Astronomique de Lyon; R. Kessler, Kavli Institute for Cosmological Physics, Chicago; and C. Baltay, A. Bauer, D. Herrera, and D. Rabinowitz, Yale University) reports that a spectrum (range 320-1000 nm) of 2006ds, obtained on July 20.5 UT with the Supernova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope, reveals that it is a type-II supernova. The spectrum exhibits H-alpha in net emission (full width at continuum of 5000 km/s), other hydrogen Balmer P-Cyg features, and P-Cygni He I 587.6-nm (7000 km/s maximum ejection velocity, measured from the blue absorption edge). The galaxy PGC 70011 is reported to have z = 0.0293 (Ratcliffe et al. 1998, MNRAS 300, 417).