[IAUC] CBET 786: 20061226 : SUPERNOVAE 2006sv-2006tc
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Electronic Telegram No. 786
Central Bureau for Astronomical Telegrams
INTERNATIONAL ASTRONOMICAL UNION
M.S. 18, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
IAUSUBS en CFA.HARVARD.EDU or FAX 617-495-7231 (subscriptions)
CBAT en CFA.HARVARD.EDU (science)
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SUPERNOVAE 2006sv-2006tc
Further to CBETs 611 and 770, B. Bassett, South African Astronomical
Observatory (SAAO); A. Becker, University of Washington (UW); H. Brewington,
Apache Point Observatory (APO); C. Choi, Seoul National University (SNU);
D. Cinabro, Wayne State University; F. DeJongh, Fermilab; J. Dembicky, APO;
D. L. DePoy, Ohio State University (OSU); B. Dilday, University of Chicago
(UC); M. Doi, University of Tokyo (UoT); J. Frieman, Fermilab and UC; P.
Garnavich, University of Notre Dame; M. Harvanek, APO; C. Hogan, UW; J.
Holtzman, New Mexico State University; M. Im, SNU; S. Jha, Stanford
University (SU); K. Konishi, UoT; J. Krzesinski, APO; H. Lampeitl, Space
Telescope Science Institute (STScI); R. Kessler, UC; B. Ketzeback, D. Long,
O. Malanushenko, and V. Malanushenko, APO; J. Marriner and D. McGinnis,
Fermilab; R. McMillan, APO; G. Miknaitis, Fermilab; T. Morokuma, UoT; R.
Nichol, University of Portsmouth (UP); K. Pan, APO; J. L. Prieto, OSU; M.
Richmond, Rochester Institute of Technology; A. Riess, STScI; R. Romani, SU;
M. Sako, University of Pennsylvania; G. Saurage, APO; D. Schneider,
Pennsylvania State University; M. Smith, UP; S. Snedden, APO; N. Takanashi
and K. Tokita, UoT; K. van der Heyden, SAAO; S. Watters, APO; C. Wheeler,
University of Texas; N. Yasuda, UoT; and C. Zheng, SU, on behalf of the
Sloan Digital Sky Survey II collaboration, report the discovery of eight
new supernovae on multiple g, r, and i images taken with the SDSS 2.5-m
telescope at APO by the SDSS observing team. Romani, Zheng, Sako, Wheeler,
and Schneider, together with U. Hopp (University of Munich) and W.
Kollatschny (University of Goettingen), report that spectroscopic
observations with the Hobby Eberly Telescope on Dec. 13, 15, and 18 UT
indicate that seven of the new objects are type-Ia supernovae and that
the eighth, 2006sz, is a probable type-Ia supernova. The discovery
magnitudes tabulated below are all SDSS g magnitudes. Spectroscopic
redshifts are given in the column labelled "z". Peak dates (all 2006) are
approximate estimates from early fits to the multi-band light curves or
from the spectra.
SN Discov. R.A. (2000.0) Decl. Mag. z Estimated
Date UT Peak Date
2006sv Nov. 9 22 25 28.25 + 0 15 55.0 22.0 0.30 Nov. 19
2006sw Nov. 14 1 05 00.20 - 0 22 28.7 22.7 0.33 Nov. 25
2006sx Nov. 16 0 31 48.32 - 0 30 50.2 21.9 0.23 Nov. 24
2006sy Nov. 16 2 21 05.20 + 0 49 42.2 22.6 0.21 Dec. 1
2006sz Nov. 16 23 42 52.46 - 0 33 22.9 22.6 0.19 Nov. 21
2006ta Nov. 19 3 29 50.42 + 0 17 42.3 22.0 0.29 Nov. 27
2006tb Nov. 19 3 45 15.49 - 0 07 42.8 22.3 0.30 Nov. 18
2006tc Nov. 23 3 08 01.96 + 0 56 36.4 22.3 0.21 Dec. 1
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2006 CBAT
2006 December 26 (CBET 786) Daniel W. E. Green
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