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 SN 2006dp (cf. CBET 574), obtained on July 13.6 UT with the Supernova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope, reveals that it is a type-II supernova. P-Cyg features from hydrogen Balmer lines, He I 587.6-nm, and the Ca II infrared triplet are visible. The maximum ejection velocity, measured from the blue wings of the H-alpha and He I 587.6-nm absorption features, is approximately 10000 km/s.