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2006CBET..397....1B - Central Bureau Electronic Telegrams, 397, 1 (2006/February-0)
No supernova 2006U.
BLANC N., COPIN Y., GANGLER E., SMADJA G., ANTILOGUS P., GILLES S., PAIN R., PEREIRA R., ALDERING G., BAILEY S., BONGARD S., KOCEVSKI D., LEE B.C., LOKEN S., NUGENT P., PERLMUTTER S., SCALZO R., THOMAS R.C., WANG L., WEAVER B.A., PECONTAL E., RIGAUDIER G., KESSLER R., BALTAY C., RABINOWITZ D. and BAUER A.
Abstract (from CDS):
The "Nearby Supernova Factory" collaboration (N. Blanc, Y. Copin, E. Gangler, 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, 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; 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 2006U (cf. IAUC 8667), obtained on Feb. 8.4 UT with the Supernova Integral Field Spectrograph on the University of Hawaii 2.2-m telescope, shows it to be an active galactic nucleus (AGN) at redshift 0.25. The redshift was determined by matching H_alpha and H_beta to the SDSS composite AGN template (Vanden Berk et al. 2001, A.J. 122, 549).
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Simbad objects: 1
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