2005CBET..304....1B -
Central Bureau Electronic Telegrams, 304, 1 (2005/November-0)
Supernovae 2005kn-2005ku.
BARENTINE J., BASSETT B., BECKER A., BREWINGTON H., DEJONGH F., DEMBICKY J., DEPOY D.L., DILDAY B., DOI M., ELSON E., FRIEMAN J., HARVANEK M., GUETH T., HOLTZMAN J., KONISHI K., LAMPEITL H. and KESSLER R.
Abstract (from CDS):
Further to CBET 254 and 281, J. Barentine, Apache Point Observatory (APO); B. Bassett, University of Portsmouth (UP); A. Becker, University of Washington; H. Brewington, APO; F. DeJongh, Fermilab; J. Dembicky, APO; D. L. DePoy, Ohio State University (OSU); B. Dilday, University of Chicago (UC); M. Doi, University of Tokyo; E. Elson, South African Astronomical Observatory (SAAO); J. Frieman, Fermilab and UC; P. Garnavich, University of Notre Dame; M. Harvanek, APO; T. Gueth and J. Holtzman, New Mexico State University; K. Konishi, University of Tokyo; J. Krzesinski, APO; H. Lampeitl, Fermilab; R. Kessler, UC; B. Ketzeback, D. Long, O. Malanushenko, and V. Malanushenko, APO; J. Marriner, Fermilab; J. L. Marshall, OSU; R. McMillan, APO; G. Miknaitis, Fermilab; T. Morokuma, University of Tokyo; R. Nichol, UP; K. Pan, APO; J. L. Prieto, OSU; M. Richmond, Rochester Institute of Technology; A. Riess, Space Telescope Science Institute; R. Romani and M. Sako, Stanford University; D. Schneider, Pennsylvania State University; M. Smith, UP; S. Snedden, APO; M. Subbarao, UC and Adler Planetarium; N. Takanashi and K. Tokita, University of Tokyo; K. van der Heyden, SAAO; and N. Yasuda, University of Tokyo, on behalf of the Sloan Digital Sky Survey II collaboration, report the discovery of eight supernovae on multiple g, r, and i images taken with the SDSS 2.5-m telescope at Apache Point Observatory by the SDSS observing team. Spectroscopy was obtained with the Hobby-Eberly Telescope, the William Herschel Telescope, the ARC 3.5-m telescope, and the MDM 2.4-m telescope, showing five of the new supernovae to be type-Ia events, two to be of type Ib/c (2005kr and 2005ks, showing broad lines similar to 1998bw), and one to be a probable type-Ia event (2005kn). The discovery magnitudes tabulated below are all g magnitudes. Spectroscopic redshifts are given in the column labelled z. Peak g magnitudes and dates (all 2005) are estimated from fits to the multi-band light curves. SN Discov. R.A. (2000.0) Decl. Mag. z Estimated Peak Date Date Mag. 2005kn Oct. 24 21 15 32.45 - 0 21 19.2 22.1 0.19 Oct. 30 21.4 2005ko Oct. 28 23 50 05.02 - 0 55 17.0 22.6 0.19 Nov. 8 21.1 2005kp Nov. 1 0 30 53.16 - 0 43 07.8 21.8 0.11 Nov. 16 19.3 2005kq Nov. 2 23 11 20.91 - 0 36 31.1 22.8 0.39 Nov. 9 21.9 2005kr Nov. 3 3 08 29.66 + 0 53 20.2 22.1 0.13 Nov. 13 20.5 2005ks Nov. 4 21 37 56.56 - 0 01 56.9 22.5 0.10 Nov. 13 21.1 2005kt Nov. 7 1 10 58.05 + 0 16 34.1 20.5 0.07 Nov. 20 18.2 2005ku Nov. 10 22 59 42.61 - 0 00 49.3 20.7 0.05 Nov. 26 17.5
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