SIMBAD references

The "Nearby Supernova Factory" group (N. Blanc, S. Bongard, 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; G. Aldering, S. Bailey, 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; C. Bonnaud and E. Pecontal, 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 2005hc, obtained on Oct. 18.5 UT with the University of Hawaii 2.2-m telescope (+ Supernova Integral Field Spectrograph), reveals that it is a type-Ia supernova on the rise, spectroscopically similar to SN 1994D at five days before maximum light. In addition to a weak Ca II infrared triplet absorption around 10000 km/s, a stronger high-velocity (20000-25000 km/s) component is visible, reminiscent of the type-Ia SN 2001el (Wang et al. 2003, Ap.J. 591, 1110).