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2006CBET..544....2A - Central Bureau Electronic Telegrams, 544, 2 (2006/June-0)
Supernova 2006cy.
ANTILOGUS P., GILLES S., PAIN R., PEREIRA R., BLANC N., COPIN Y., GANGLER E., SMADJA G., ALDERING G., ARAGON C., BAILEY S., BONGARD S., CHILDRESS M.J., KOCEVSKI D., LOKEN S., NUGENT P., PERLMUTTER S., RUNGE K., SCALZO R., THOMAS R.C., WANG L., WEAVER B.A., PECONTAL E., RIGAUDIER G., KESSLER R., BALTAY C., BAUER A., HERRERA D. and RABINOWITZ D.
Abstract (from CDS):
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 2006cy, obtained on June 10.4 UT with the Supernova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope, reveals it to be a type-IIn supernova, exhibiting narrow emission features from H-alpha through H-delta, and also He I 587.6-, 667.8-, and 706.5-nm.
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